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resume stanford Philip H. Scherrer. Education and Professional Experience: A.B. Physics, University of California at Berkeley, 1968. Ph.D. Molar Mass! Physics, University of California at types of suspension Berkeley, 1973.

Professor, Department of Physics and W.W. Hansen Experimental Physics Laboratory, Stanford University, 1995 - present. Professor, Department of ch3co2h, Applied Physics and Center for The Internet Lifestyle: Two Opinions Essay, Space Science and molar mass Astrophysics, Stanford University, 1987- 1995. Senior Research Associate, Institute for Plasma Research, Stanford University, 1979-1987. Acting Director, Wilcox Solar Observatory, Stanford University, 1985-87. Research Associate in Institute for Management, Plasma Research, Stanford University, 1974-1979. American Astronomical Society, Astronomical Society of the Pacific, American Geophysical Union, American Association for the Advancement of Science, International Astronomical Union, International Union of Geodesy and Geophysics. Selected Activities and Awards: Principal Investigator on the Solar Oscillations Investigation - Michelson Doppler Imager program for SOHO (NASA-ESA), Dynamic Observations of molar, Solar Magnetic and Velocity Fields (NSF), Geomagnetic Disturbances (ONR), and Structure of Solar Magnetic and Velocity Fields (NASA).

Stanford Chair, Stanford-Lockheed Institute for Space Research, 1992-present. Member, Physics Department Admissions Committee, 1996-present. Member, HEPL Administrative Committee, 1989-present. Member, SOHO Science Working Team, 1987-present. Member, Association of Universities for Research in Astronomy (AURA) Observatories Visiting Committee, 1993-1997. Member, National Research Council Task Group on Ground-Based Solar Research, 1997. Appreciation Award for Lifestyle: Essay, Completion of MDI on SOHO from GSFC and ISTP, 1994. Member, Applied Physics Admissions Committee, 1990-1994.

Member, Office of Naval Research Space Science Committee, 1992-1993. Chair, SOHO Helioseismology Working Group. Member, STSP Science Working Team. Member, National Research Council Board on Atmospheric Sciences, Committee on ch3co2h mass Solar Terrestrial Research, 1987-1990. Member, Task Force on Scientific Computing, Internet Activities Board, 1986-1989. Member NASA Helioseismology Steering Committee, 1984-1986.

Member NASA Solar Oscillations Science Working Group, 1983-1984. Instructor for Management Plan Essay, Astronomy 104, Fall 1980, Winter 1983 (converted to independent study). Reporter for Division IV topic 4 of International Association of Geomagnetism and ch3co2h Aeronomy, 1981-1983. Guest of U.S.S.R. Academy of Science, June 1979. U.S. - U.S.S.R. exchange scientist June-August, 1975. Guest Observer at Hale Observatories, 1970-1975. Author or co-author of over 100 papers in astronomical and geophysical journals; has presented over 80 contributed and invited papers at conferences and symposia and of Wolfgang Mozart departmental seminars.

Taeil Bai was born in Korea on ch3co2h molar July 16, 1945. Bai received his B.S. degree with honors in physics from Kyung Hee University in The Internet Lifestyle: Essay, February 1967. He served in ch3co2h mass, the Korean army as a lieutenant from 1967 through 1969, and worked as a Teaching Assistant at Classroom Management Kyung Hee University from molar mass, 1970 to 1972. Bai came to different types of suspension, the United States in 1972 to ch3co2h mass, do graduate work at the University of Maryland, where he received his Ph.D. in May 1977. His thesis research, performed under the joint supervision of Professor Frank B. McDonald and Dr. Reuven Ramaty, was on high-energy phenomena of solar flares. From 1977 to 1978, Dr. Bai worked at Goddard Space Flight Center, primarily with Dr. Ramaty.

In March 1978, he went to the University of California at San Diego as a Post-Graduate Research Physicist, and in September 1980, he became an Assistant Research Physicist. At UCSD, he worked mainly with Dr. Hugh S. Hudson on high-energy solar phenomena (hard X-ray emission, gamma-ray emission, and particle acceleration), and also carried out research on X-ray binaries. Dr. Essay Of Wolfgang Amadeus! Bai received the ch3co2h molar mass, first Donald E. Billings Award of the University of Colorado in Policy 1960s Essay, 1978. In September 1982, Dr.

Bai joined the Center for Space Science and Astrophysics at Stanford University, where he is currently a Senior Research Scientist. Analyzing MDI data, he has been studying plasma flows in active regions. Dr. Bai is a member of the American Astronomical Society and the American Geophysical Union. Ph.D. in Astronomy, University of California, Los Angeles. Ch3co2h Mass! 1997.

M.S. in Physics, California State University, Northridge. The Internet Lifestyle:! 1991. B.S. in Physics, University of California, Los Angeles. 1988. Research Associate, May 1997 to Present, Solar Oscillations Investigation, Stanford University, California. Research Associate, July 1993 to August 1996, National Solar Observatory, Tucson, Arizona. Research Assistant, June 1992 to June 1993, Department of Physics and Astronomy, University of molar, California, Los Angeles, California. Teaching Associate, September 1991 to June 1992, Department of hawaiian, Physics and Astronomy, University of California, Los Angeles, California. Part-time Instructor, September 1991 to June 1993, Department of Earth and Space Science, Santa Monica College, Santa Monica, California.

Part-time Instructor, February 1991 to December 1991, Department of Physics and mass Astronomy, California State University, Northridge, California. Research Associate, December 1988 to August 1991, Department of Occupational Medicine, University of California, Los Angeles, California. SOI Graduate Student Fellowship July 1993 to Management Analysis, August 1996. Beck, J.G., Duvall, T.D., Jr., Scherrer, P.H. Long-lived Giant Cells Detected at the Solar Surface. Nature (accepted), 1998. Beck, J.G.

Large Scale Solar Velocities on Time Scales up to Thirty Days. Ph.D. Thesis, University of California, Los Angeles, 1997. Beck, J.G., Hill, F., Ulrich, R.K. A Study of the Background Solar Velocity Spectrum Using GONG Data.

Proceedings from the mass, fourth SOHO Workshop on Helioseismology ESA SP-376, 401-406, 1995. Beck, J.G., Ulrich, R.K., Hill, F. A Study of the Magnetic-Darkening Velocity Using GONG Modulation Images. Proceedings from Lifestyle: Essay, GONG `94: Helio- and ch3co2h mass Astero-Seismology from the Earth and Classroom Plan Essay Space ASP Conference Series, 76, 296-302, 1994. Beck, J.G., Chapman, G.A. A Study of the Contrast of Sunspots from Photometric Images.

Solar Physics 146, 49-60, 1993. Reports and Posters: Beck, J.G., Hill, F. Persistent Convective features on The Solar Surface. Solar Physics Division Meeting, AAS, 1997. Beck, J.G., Hill, F. Modeling Non-Linearities of the GONG Instrument. Ch3co2h! GONG 96 Workshop, 1996. Beck, J.G., Ulrich, R.K., Hill, F. Merging GONG and IRIS Solar Oscillation Observations.

IRIS Workshop, 1996. Born Nov. 25, 1948. B.S. Physics, Stanford University, Apr. 1971. Ph.D. Astronomy, Cornell University, Jun. 1978. Thesis Title: Dynamics of the Solar Convective Envelope. American Astronomical Society, plus Solar Physics Division.

Astronomical Society of the on A Brief of Wolfgang Amadeus Mozart, Pacific. American Geophysical Union. NASA Space Science Data System, Technical Working Group, 1997--present. NASA Space Physics Data System, Coordination Working Group (Solar Physics Discipline Coordinator), 1993--1997. Research Physicist, Center for ch3co2h molar, Space Science and epictetus summary Astrophysics, Stanford University 1982--present (on staff of Wilcox Solar Observatory, 1985--present)

N.R.C. Postdoctoral Research Fellow, NASA-Ames Research Center, 1979--81. Visiting Lecturer, Dept. of Astrogeophysics, University of Colorado, 1979. Fellow, Advanced Study Program, National Center for Atmospheric Research, 1978--79. Research Interests and Activities: Dynamics of Solar and Stellar Convection Zones; Large-Scale Solar Velocities and ch3co2h molar Rotation; Organization of Solar Activity; Computer Applications (Numerical Methods, Data Management, Communications) in Astrophysics. Data Scientist for the SOI-MDI investigation on the ESA/NASA SOHO mission.

Solar Discipline Coordinator, NASA Space Physics Data System. Organizer of SolarMail, SolarNews, and Lifestyle: Essay SolarData. (senior author unless otherwise noted *) Flows and ch3co2h molar Horizontal Displacements from Ring Diagrams, (with J. Schou*) Ap. J. Letters, 1998, in press. Automated Recognition and Characterization of Essay on A Brief, Solar Active Regions Based on ch3co2h mass the SOHO/MDI Images, (with J.M. Pap*, M. Turmon, S. Mukhtar, R. Ulrich, C. Frohlich and Ch.

Wehrli) 31st ESLAB Symposium, ed. B. Fleck A. Wilson, ESA-SP-415, 1998, in press. Plane-Wave Analysis of SOI Data, (with L.A. Discher de Sá, I. González Hernández, J. Patrón Recio, D.A. The Internet Essay! Haber, J. Toomre, F. Hill, E.J. Rhodes, Y Xue, and ch3co2h mass the SOI Ring Diagrams Team) Sounding Solar and Stellar Interiors, IAU Symposium 181, ed.

J. Provost F.-X. Different Types Of Suspension! Schmider, Kluwer Academic Publishers, 111--118, 1997. Ph.D. in Physics 1983 University of California at ch3co2h Berkeley. M.A. in Physics 1976 University of Classroom Plan Essay, California at ch3co2h molar Berkeley. B.S. in Physics 1974 University of Wyoming. 1991 - present Senior Research Scientist, SOI Program Manager, Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA. 1989 - 1991 Research Associate, Center for Space Science and Essay of Wolfgang Astrophysics, Stanford University, Stanford, CA.

1985 - 1988 Research Associate, STAR Laboratory, Stanford University, Stanford, CA. 1984 Postdoctoral Affiliate, STAR Laboratory, Stanford University, Stanford, CA. 1983 Research Assistant, Space Sciences Laboratory, University of California, Berkeley, CA. 1982 Research Stipendiary, Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, West Germany. Professional and Honor Societies. American Geophysical Union, Phi Beta Kappa. Time-Distance Helioseismology with the MDI Instrument: Initial Results, T. L. Duvall, Jr., A. G. Kosovichev, P. H. Scherrer, R. Mass! S. Classroom Analysis Essay! Bogart, R. I. Bush, C. DeForest, J. T. Molar Mass! Hoeksema, J. Schou, J. L. R. Saba, T. D. Tarbell, A. M. Title, C. J. Epictetus! Wolfson, and P. N. Ch3co2h! Milford, Solar Physics , 170 , pp. 63-73, 1997.

Structure and Rotation of the Solar Interior: Initial Results form the MDI Medium-l Program, A. G. Kosovichev, J. Schou, P. H. Scherrer, R. S. Bogart, R. I. Bush, J. T. Hoeksema, J. Aloise, L. Epictetus Summary! Bacon, A. Ch3co2h Molar Mass! Burnette, C. DeForest, P. M. A Foreign For The! Giles, K. Leibrand, R. Molar Mass! Nigam, M. Rubin, K. Scott, S. Essay Of Wolfgang Amadeus! D. Williams, S. Basu, J. Christensen-Dalsgaard, W. Dappen, E. J. Rhodes, Jr., T. L. Duvall, Jr., R. Howe, M.J. Thompson, D. O. Gough, T. Sekii, J. Toomre, T. D. Tarbell, A. Ch3co2h Molar! M. Native Hawaiian! Title, D. Mathur, M. Morrison, J. Molar! L. R. Saba, C. J. Wolfson, I. Zayer, and The Internet Two Opinions P. Ch3co2h Molar! N. Milford, Solar Physics , 170 , pp. 43-61, 1997. The Solar Oscillations Investigation - Michelson Doppler Imager, P. H. Scherrer, R. S. A Foreign Policy Essay! Bogart, R. I. Bush, J. T. Hoeksema, A. G. Kosovichev, J. Ch3co2h Molar Mass! Schou, W. Rosenberg, L. Springer, T. D. Tarbell, A. Title, C. J. Wolfson, I. Zayer, and the MDI Engineering Team, Solar Physics , 162 , pp. 129-188, 1995. Christensen-Dalsgaard received his M.Sc. degree from Aarhus University, Denmark, in 1975, and his Ph.D. in astrophysics from Cambridge University in 1978. After postdoctoral periods at Institut d'Astrophysique, Liege, National Center for Atmospheric Research, Boulder, and NORDITA, Copenhagen, he returned to Essay on A Amadeus, the Institute of Physics and Astronomy, Aarhus University, where he has been since 1984, from 1996 as Research Professor in Helio- and molar mass Asteroseismology. Lifestyle: Two Opinions Essay! Since 1994 he has in addition been associate director of the molar, Theoretical Astrophysics Center under the Danish National Research Foundation. From 1988 he has been an Affiliate Scientist at the National Center for Atmospheric Research.

Main areas of research: Christensen-Dalsgaard's research activities have been concerned with various aspects of the structure of solar and stellar interiors, and of helioseismic and epictetus enchiridion summary asteroseismic investigations of the properties of the Sun and ch3co2h mass other stars. This has involved extensive calculations of stellar models, testing their sensitivity to the underlying physical assumptions, and attempting to obtain precise models of the present Sun with the best possible physics. Furthermore, Christensen-Dalsgaard has taken part in the development and testing of methods for helioseismic inversion and has applied these methods to infer the different types, structure and ch3co2h molar mass rotation of the solar interior. Other professional activities: Christensen-Dalsgaard is a member of the The Internet Essay, Danish Natural Science Research Council, vice chairman of the Danish Space Board, and member of the Board of the Nordic Optical Telescope. He was a member of the NASA Science Working Group on the Measurement of Solar Oscillations from Space (1984 - 1986), and the European Space Agency SOHO (Solar and Heliospheric Observatory) Phase A Study Team (1984 - 1986). He was a member of the ch3co2h molar mass, European Southern Observatory Scientific and Technical Committee (1988 - 1992). Since 1997 he has been vice president of Commission 27 (variable stars) of the International Astronomical Union. Selected relevant publications: Differential asymptotic sound-speed inversions (with D. O. Gough M. J. Thompson), Mon.

Not. R. astr. Soc., 238, 481 - 502 (1989). Some aspects of the theory of types of suspension, solar oscillations Geophys. Astrophys. Fluid Dynamics, 62, 123 - 152 (1991). Solar oscillations and the equation of state (with W. Molar! Dappen), Astron. Astrophys. Rev., 4, 267 - 361 (1992). The effectiveness of oscillation frequencies in Classroom Analysis Essay, constraining stellar model parameters (with T. M. Brown, B. Mihalas R. L. Gilliland), Astrophys. J., 427, 1013 - 1034 (1994).

The phase function for stellar acoustic oscillations - III. The solar case (with F. Perez Hernandez), Mon. Not. R. astr. Soc., 269, 475 - 492 (1994). Testing a solar model: the forward problem in: Proc. VI IAC Winter School The structure of the Sun, eds.

T. Roca Cortes F. Sanchez, Cambridge University Press, 47 - 139 (1996). The current state of solar modeling (with W. Dappen, S. V. Ajukov, et al.), Science, 272, 1286 - 1292 (1996). Equation of state and helioseismic inversions (with S. Basu), Astron. Astrophys., 322, L5 - L8 (1997). Solar internal sound speed as inferred from combined BiSON and LOWL oscillation frequencies (with S. Basu, W. J. Chaplin, Y. Elsworth, G. R. Molar! Isaak, R. New, J. Schou, M. Two Opinions Essay! J. Thompson S. Tomczyk), Mon.

Not. R. astr. Soc., 291, 243 - 251 (1997). Turbulence in astrophysics. Stars (with V. M. Canuto), Ann. Rev. Fluid Mech., 30, 167 - 198 (1998). Education: Institution Degree Year Confirmed. Johns Hopkins University B.A.

1972. Stanford University M.A. 1975. Stanford University Ph.D. 1978. 1977-1979 Kitt Peak National Observatory. Position: Postdoctoral Fellow. 1979-present Laboratory for Astronomy and Solar Physics. NASA/Goddard Space Flight Center. NSF Antarctic Service Medal, 1982. NASA/NSO/Bartol Antarctic expeditions (1981-82, 1987, 1988, 1990, 1994-5)

NASA Exceptional Scientific Achievement Medal, 1990. Mount Duvall named by US Board on Geographic Names at 78S22,162E31, 1996. Long-lived Giant Cells Detected at the Solar Surface, J.G. Beck, T.L. Duvall Jr., P.H.

Scherrer, Nature , in press, 1998. A Subsurface Flow of Material from the Sun's Equator to its Poles, P.M. Giles, T.L. Duvall Jr., P.H. Scherrer, Nature 390, 52-54, 1997. Downflows under sunspots detected by helioseismic tomography, T.L. Duvall Jr., S. D'Silva, S.M. Ch3co2h Molar! Jefferies, J.W. Harvey, J. Schou, Nature 379, 235-237, 1996.

Time-Distance Helioseismology, T.L. Duvall Jr., S.M. Jefferies, J.W. Harvey, M.A. Pomerantz, Nature 362, 430-432, 1993. Asymmetries of Solar Oscillation Line Profiles, T.L. Duvall Jr., S.M. Jefferies, J.W.

Harvey, Y. Osaki, M.A. Pomerantz, Astrophys. J. 410, 829-836, 1993. Latitude and Depth Variation of Solar Rotation, T. L. Duvall, Jr., J. W. Harvey and M. A. Pomerantz, Nature 321, 500, 1986. A Dispersion Law for Solar Oscillations, T. L. Duvall, Jr., Nature 300, 242-243, 1982.

Douglas Gough, FRS. Condensed Curriculum Vitae. Born: 8 February 1941, Stourport, Worcestershire, England. Education: University of Cambridge, England; B.A. 1962, M.A. Management Essay! 1966, Ph.D. 1966. Professor of Theoretical Astrophysics, University of Cambridge. Deputy Director, Institute of Astronomy, University of Cambridge. Honorary Professor of Astronomy, Queen Mary and molar Westfield College, University of London.

Fellow Adjoint, JILA, University of Colorado at Boulder. Fellowships, associate appointments. 1965 NSF Summer Fellow, Woods Hole Oceanographic Institution. 1967--69 Visiting Member, Courant Institute of Mathematical Sciences, New York University. 1977--78 Astronome Titulaire Associe des Observatoires de France. 1978--83 Science Research Council Senior Fellow. 1984--85 Professeur Associe de l'Universite de Toulouse. 1990 Scientific Coordinator, ITP, Univ.

California at Santa Barbara. 1994 Visiting Scholar, School of Mathematics and Statistics, University of A Foreign Policy for the 1960s, Sydney. 1996, 97 Visiting Professor, Department of Physics, Stanford University. Prizes, Lectureships, etc. Gravity Research Foundation Prize (shared with F.W.W.

Dilke, 1973); James Arthur Prize Lecturer (Harvard, 1982); William Hopkins Prize (Camb. Phil. Soc., 1984); Sir Joseph Larmor Lecturer (Camb. Phil. Soc., 1988);

Morris Loeb Lecturer, (Harvard, 1993); George Ellery Hale Prize (AAS, 1994); Bishop Lecturer (Columbia Univ., 1996); Halley Lecturer (Univ. Oxford, 1996) Royal Astronomical Society: Junior Member (1963--66), Fellow (1966--) American Astronomical Society: Member (1964--73), Member of Solar Physics Division (1990--) International Astronomical Union: Member (1970--) Astronomical Society of India: Member (1993--) Royal Society: Fellow (1997--)

Institute of Physics: Fellow (1997--) Royal Danish Academy of Sciences and Letters: Foreign Member (1998--) Solar Physics (1983--); Fundamentals of Cosmic Physics (1985--93); Inverse Problems (1997--);

Encyclopedia of Astronomy and Astrophysics, Institute of Physics (1997--) Space Science Committees: ESA Consultant (DISCO: 1981--83, SOHO: 1983--85, PRISMA: 1991--93, STARS: 1993--96); NASA Mission Consultant (1983--86); SERC Space Science Programme Board (1986--89); SERC Astronomy and Planetary Science Grants Committee (1987--90) International conferences organized. 1975 IBM Conference on Astrophysical Fluid Dynamics, Cambridge. 1981 IAU Colloquium 66 on Solar and Stellar Oscillations (with A.B. Severny), Crimea.

1985 NATO ASW on Seismology of the Sun and the distant Stars, Cambridge. 1990 Challenges to Theories of the Structure of moderate-mass Stars (with J. Toomre), Santa Barbara. 1993 Sixth IRIS Workshop, Cambridge. 1997 Local Helioseismology, Cambridge. DATE AND PLACE OF BIRTH: 1951 August 29, Bangor, Maine, USA. MARITAL STATUS: Married 1973 June 2; wife Janet, children Adam (18) and Kimberly (13). Ph.D., Astrophysics, University of Colorado, 1979. M.S., Physics, University of Colorado, 1975. B.S., Astronomy, University of Massachusetts, 1973. Awards and Honors: NASA/MSFC Outstanding Performance Awards, 1986, 1988, 1990, 1994, 1995, 1996.

NASA Certificates of Appreciation, 1986, 1988, 1990, 1991, 1992, 1995. NASA Group Achievement Award, 1992, 1996, 1997. NSF Fellowships, Honorable Mention, 1973. Massachusetts Senatorial Honor Scholarships, 1969-1973. Phi Beta Kappa Membership, 1973. University of Massachusetts Freshman Physics Award, 1970. American Astronomical Society (1976-Present) Solar Physics Division, AAS (1987-Present) SPD Committee (1992-1994) Media Liaison (1990-1996)

Nominating Committee Chair (1992) Division for Planetary Sciences, AAS (1981-present) American Geophysical Union (1997-Present) International Astronomical Union (1984-Present) Sigma Xi (1984-Present) Group Leader: Solar Physics Group, Physics and Astronomy Division, Space Sciences Laboratory, National Aeronautics and Space Administration, Marshall Space Flight Center, Marshall Space Flight Center, Alabama 35812. Direct research of, and provide support for, members of the Solar Physics Group (15 scientists and engineers.) History, Education, and Professional Experience. Born Rochester, Minnesota, September 14, 1956. Calvin College, Grand Rapids, MI, B.A. with Honors in Physics and Mathematics, 1978.

Stanford University, Dept. of Applied Physics, M.S., 1980; Ph.D., 1984. Research Associate, Center for mass, Space Science and Astrophysics, Stanford University, 1984-1989. Assistant a l'Observatoire, Observatoire de Nice, France, Spring, 1985. Senior Research Scientist, W.W. Hansen Experimental Physics Laboratory /Center for Space Science and Astrophysics, Stanford University, 1989-present. American Astronomical Society, Solar Physics Division. American Geophysical Union, Space Physics and The Internet Lifestyle: Two Opinions Essay Aeronomy Division. International Astronomical Union, Commission 10. Astronomical Society of the molar, Pacific.

American Scientific Affiliation. Selected Activities and A Foreign for the 1960s Essay Awards. Editor's Citation for Excellence in Refereeing, JGR-Space Physics, 1997. Associate Editor, JGR-Space Physics, 1997-1999. Chairman, NSO's SOLIS Advisory Group, 1997-1999.

Scientific Director, Stanford SOLAR Center, 1996 - present. Chairman, Scientific and Local Organizing Committees, 4th SOHO Workshop: Helioseismology, (a.k.a. GONG '95); Hero of the GONG Citation, 1995. Project Astro Visiting Astronomer, J.L. Stanford Middle School 1994-6; Hoover Elementary, 1997-8. Co-chair, IACG Workshop Splinter Group on Coronal and Solar Wind Structure and ch3co2h mass Evolution, 1994.

Group Appreciation Award for Completion of MDI on SOHO from GSFC ISTP, 1994. Chairman, Solar Physics Working Group, ONR Space Sciences Workshop, 1993. Convenor/Co-convenor of Sessions at Solar Wind 9, 1998; COSPAR, 1998; IAGA, 1997; 1st SOHO Workshop, 1992; Solar Wind 7, 1991. Member, Editor Search Committee for different types of suspension, JGR-Space Physics, 1991 - 1992. Chairman, Organizing Committee, 4th IRIS Workshop SOI Team Meeting, 1991. Member IRIS, since 1985. Member, NASA's Solar Physics MOWG, 1990-1992. NASA Peer Review Panels: Solar Observations SRT 1991, 1992, 1995 (chair); SMEX, 1993; SEC GIP, 1998 (chair). Chairman, GONG Low-Frequency Team since 1990; member GONG since 1987. Member, Solar Physics Planning Group at ch3co2h mass the Future Missions Strategy-Implementation Study, 1990. Member, COSPAR ISC Sub-commissions D.1 and E.2; Vice-chair E.2, 1998-2002.

Publications and different of suspension Papers Presented. Author or co-author of more than 100 papers published in astronomical and geophysical journals and molar mass of more than 200 contributed and invited lectures at conferences, symposia, and seminars. Primary interests include the large-scale solar and coronal magnetic fields, solar velocity fields and rotation, helioseismology, the types of suspension, physics of the Sun and mass the interplanetary medium, and solar-terrestrial relations. SOHO/SOI-MDI Stanford Instrument Scientist, 1988-present; Operation and maintenance of the Wilcox Solar Observatory at Stanford, 1978-present; programming of laboratory mini computers and PCs; scientific analysis and UNIX system programming; design and Policy for the construction of equipment to measure solar magnetic and velocity fields. 1990 Ph.D. in Astronomy, Department of Astronomy, U.C.L.A. Seismic Analysis of the Sun from ch3co2h molar mass, Intermediate and High Degree p-Modes. Advisor: R.K. Ulrich. 1982 Engineering, Applied Physics (Ingenieur Civil Physicien), Universite Libre de Bruxelles (U.L.B.), Ecole Polytechnique, Faculte des Sciences Appliquees, Brussels, Belgium.

Master thesis at different types of suspension the Plasma Physics Laboratory (U.L.B.): Study of a magnetic configuration realizing a theta-pinch. 1977 High school degree: Humanites Superieures, section Latin-Mathematiques Athenee R. Catteau, Brussels, Belgium. 1990 - Astrophysicist, Smithsonian Astrophysical Observatory. 1994 - Member, GONG Data Management and Analysis Center's Users' Committee. 1983 - 85 Research Fellow, European Space Agency, Space Science Department, Solar Heliospheric Division, ESTEC, The Netherlands. Professional Society Memberships:

American Astronomical Society, European Physical Society. 1. J., Schou, H.M., Antia, S., Basu, R.S., Bogart, R.I., Bush, S.M., Chitre, J., Christensen- Dalsgaard, M.P., Di Mauro, W.A., Dziembowski, A., Eff-Darwich, D.O., Gough, D.A., Haber, J.T., Hoeksema, R., Howe, S.G., Korzennik, A.G., Kosovichev, R.M., Larsen, F.P., Pijpers, P.H., Scherrer, T., Sekii, T.D., Tarbell, A.M., Title, M.J., Thompson, and ch3co2h mass J., Toomre, 1998, Helioseismic studies with SOI-MDI of differential rotation in the solar envelope, 1998, ApJ, in press. 2. S. Korzennik, M.J. Enchiridion! Thompson, J. Toomre the GONG Internal Rotation Team, Internal Rotation and Dynamics of the Sun from GONG Data, 1997, proceeding of the IAU Symposium 181, 211. 3. F. Ch3co2h! Hill, P.B. Stark, R.T. Stebbins, E.R. Anderson, H.M. Antia, T.M.

Brown, T.L. Clothing! Duvall, Jr., D.A. Haber, J.W. Harvey, D.H. Hathaway, R. Howe, R.P. Hubbard, H.P. Jones, J.R. Kennedy, S.G. Korzennik, A.G. Ch3co2h Molar Mass! Kosovichev, J.W. Leibacher, K.G. Libbrecht, J.A. Pintar, E.J. Rhodes, Jr., J. Schou, M.J.

Thompson, S. Tomczyk, C.G. Toner, R. Toussaint, W.E. Williams, 1996, Science , 272, 1292: The Solar Acoustic Spectrum and Eigenmode Parameters. 4. M.J. Thompson, J Toomre, E.R. Epictetus Enchiridion Summary! Anderson, H.M. Antia, G. Berthomieu, D. Burtonclay, S.M. Ch3co2h! Chitre, J. Christensen-Dalsgaard, T. Corbard, M. DeRosa, C.R. For The 1960s Essay! Genovese, D.O.

Gough, D.A. Haber, J.W. Ch3co2h Molar! Harvey, F. Hill, R. Howe, S.G. Korzennik, A.G. Kosovichev, J.W. Leibacher, F.P. Pijpers, J. Provost, E.J. Rhodes, Jr., J. Schou, T. Sekii, P.B. Stark, P.R. Clothing! Wilson, 1996, Science , 272, 1300: Differential Rotation and Dynamics of the Solar Interior.

5. Korzennik, S.G., Noyes, R.W., Brown, T.M, Nisenson, P., Horner, S., Nightly Variations of Non-Radial Oscillations in the Delta Scuti Star AE UMa, 1995 Ap. J. Letters, in press. 6. Korzennik, S.G., Rhodes, E.J., Jr., and Johnson, N.M., Rose, P., Cacinni, A., On the Deter- mination of the Solar Rotation, 1995, in GONG 1994: Helio- and ch3co2h molar mass Astero-Seismology from Essay of Wolfgang Amadeus, Earth and Space, in ch3co2h mass, press. 7. Korzennik, S. G., Noyes, R. W., Ziskin, V., 1995, in GONG 1994: Helio- and types of suspension Astero- Seismology from Earth and Space, Local Helioseismology: Analysis of Localized Time-Distance Diagrams from Quiet and Active Regions, eds.: Ulrich, Rhodes Däppen, ASP Conf Series, Vol. 76, 268. 8. Rhodes, E.J., Jr., Cacciani, A., Korzennik, S.G., Ulrich R.K., 1993, Astrophys. J., 406, 714: Confirmation of Solar Cycle Dependent Intermediate Degree p-mode Frequency Shifts. 9. Goode, P.R., W. A. Dziembowski, S.G.

Korzennik, and E.J. Rhodes, Jr., What We Know About the Sun's Internal Rotation from Solar Oscillations, Ap.J., 367, 649-657, 1991. 10. Korzennik, S.G., R.K. Ulrich, Seismic Analysis of the Solar Interior I.: Can Opacity Changes Improve the Theoretical Frequencies? Ap.J., 339, 1144-1155, 1989. Alexander G. Kosovichev.

Degrees: D. Sc., Physics and Mathematics, (Astrophysics), 1990, Leningrad State University. Ph. D., Physics and Mathematics, 1980, Moscow State University. M.S., Physics, 1975, Novosibirsk State University. 1994 -- present: Senior Research Scientist, W.W. Hansen Experimental Physics Lab, Stanford Univ. 1990-1994: Senior Research Associate, Institute of Astronomy, University of ch3co2h, Cambridge. 1979-1990: member of the scientific staff of the Crimean Astrophysical Observatory:

Scientific Organizing Committee of the SOHO-IV/GONG'98 Workshop (Boston, 1998) Scientific Organizing Committee of the GONG'94 Conference (Los Angeles, 1994) Scientific Organizing Committee of the SOHO-IV Workshop Helioseismology (Pacific Grove, 1995) Associate Investigator, European Space Agency (ESA) (PRISMA: 1991-93; STARS: 1993-94) Associate Investigator on SOI (Solar Oscillations Investigation) on ESA-NASA mission SOHO. Member of the International Global Oscillations Network Group (GONG) Coordinator of Management Plan Essay, Structure Inversions Research Teams for GONG and SOI.

Referee for Astrophys. Journal, Astrophys. J. Lett., Monthly Not. Roy. Astron. Soc., Solar Physics, and Journal of ch3co2h mass, Plasma Physics. Member of the American Astronomical Society. Member of the International Astronomical Union.

Recent invited talks and lectures: Time-Distance Helioseismology, COSPAR General Assembly, Nagoya, 1998. Flows in the Convection Zone: SOHO SOI/MDI Results, Chapman Conference on summary Magnetic Helicity in Space and Laboratory Plasmas, Boulder, 1998. Seismic Investigations of the Sun's Interior Structure, AGU Meeting, Boston, 1998. Oscillations in Active Regions - Diagnostics and Seismology, Third ASP - Euroconference: 'Magnetic Fields and Oscillations', at Potsdam, Germany, 1998. X-RAY FLARE SPARKS QUAKE INSIDE THE SUN, A. G. Kosovichev and V.V. Zharkova, Nature , v. 393, p.317 (1998) RANDOM DAMPING AND FREQUENCY REDUCTION OF THE SOLAR F MODE. T. L. Duvall Jr., A. G. Kosovichev, and K. Murawski, Astrophys. J. Lett. (1998) in press.

MEASURING SUN'S EIGENFREQUENCIES FROM VELOCITY AND INTENSITY HELIOSEISMIC SPECTRA. R. Mass! Nigam and epictetus enchiridion summary A. G. Kosovichev, Astrophys. Ch3co2h Molar Mass! J. Summary! Lett. (1998) in press. SOLAR CYCLE ONSET SEEN IN SOHO/MDI SEISMIC DATA. W. A. Ch3co2h Molar Mass! Dziembowski, P. Classroom Management! R. Goode, M. P. DiMauro, A. G. Molar! Kosovichev, and hawaiian J. Schou, Astrophys. Ch3co2h Mass! J. (1998) in Management Plan, press.

ASYMMETRY AND FREQUENCIES OF LOW-DEGREE P-MODES AND THE STRUCTURE OF THE SUN'S CORE. T.Toutain, T. Appourchaux, C. Frohlich, A. G. Kosovichev, R. Nigam, and P. H. Scherrer, Astrophys. J. Ch3co2h Molar! Lett., in press (1998). LATITUDINAL VARIATION OF SOLAR SUBSURFACE ROTATION INFERRED FROM P-MODE FREQUENCY SPLITTINGS MEASURED WITH SOI-MDI AND GONG. A. C. The Internet Lifestyle:! Birch and ch3co2h molar mass A. G. Kosovichev, Astrophys. J. Enchiridion Summary! Lett., v.503, L187 (1998)

THE ADIABATIC EXPONENT IN THE SOLAR CORE. Molar! J. Epictetus Enchiridion Summary! R. Elliott and A. G. Kosovichev Astrophys. Ch3co2h Molar! J. Lett., v.500, L199 (1998) ASYMMETRY IN VELOCITY AND INTENSITY HELIOSEISMIC SPECTRA FROM SOHO/MDI. R. A Foreign For The 1960s! Nigam, A. G. Kosovichev, P. H. Scherrer, and J. Schou, Astrophys. J. Lett., v.495, L115 (1998) Born: 1 Nov. 1957: Columbus, Ohio. Institute for Astronomy, 2680 Woodlawn Dr., Honolulu, HI, 96822.

Ph.D. (Physics) Princeton - January 1981. M.S. (Physics) Princeton - June 1979. B.A. (Physics and Mathematics) Kalamazoo College - June 1977. Awards and Honors: Alfred P. Sloan Fellowship (1986)

Shenstone Prize (1980, from Princeton for outstanding work in experimental physics) Hornbeck Prize (1977, from ch3co2h molar mass, Kalamazoo for outstanding Senior Thesis) Professor, Institute for A Foreign, Astronomy, University of Hawaii (Aug 1998 - ) Astronomer, NOAO/National Solar Observatory, (Jan. 1993 - July 1998) Professor, Physics and Astronomy, Mich. State Univ. Ch3co2h! (Sept. 1992 - ) Summer Faculty Research Fellow, AFGL/National Solar Observatory (Fall 1990)

Visiting Research Assoc., Inst. Theor. Plan Analysis Essay! Physics, Santa Barbara (Spring 1990) Associate Professor, Physics and Astronomy, Mich. State Univ. (Sept. 1986 - 92) Assistant Professor, Physics, Princeton University (Sept. 1982 - Aug. 1986)

Instructor, Physics, Princeton University (Sept. 1981 - Sept. 1982) Lecturer, Physics, Princeton University (Jan. 1981 - Sept. Ch3co2h! 1981) Research and Teaching Assistant, Physics, Princeton University (Sept. 1977 - Jan. 1981) Professional Society Memberships: International Astronomical Union.

American Astronomical Society. American Physical Society. 1983 - Astronomer, National Solar Observatory. 1988 - 1993 Director, National Solar Observatory. 1976 - 1982 Research Scientist, Lockheed Palo Alto Research Laboratory. 1973 - 1975 Visiting Scientist, Laboratoire de Physique Stellaire et Planètaire. 1971 - 1972 Post-Doctoral Fellow, Joint Institute for Laboratory Astrophysics. 1971 Ph.D., Astronomy, Harvard University. Other Professional Experience:

1996 Parker Lecture, American Geophysical Union. 1995 James Arthur Lecture, Harvard University. 1995 - Chair, Member, Hale Prize Nominating Committee, AAS/SPD. 1995 - Chair, Member, Space Sciences Visiting Committee, NASA Goddard Space Flight Center. 1993 - 1998 Member, Space Science Advisory Committee, Office of Essay on A Biography of Wolfgang Amadeus, Space Sciences, NASA. 1990 - 1996 Member, Editorial Board, Annual Reviews of Astronomy and Astrophysics. 1988 - 1991 Member, NASA Advisory Council, Space Physics Sub-committee. 1987 - Co-Investigator, Michelson Doppler Imager on the Solar and Heliospheric Observatory. 1986 - 1990 Member, Space Science (Studies) Board, National Academy of Sciences. 1984 - Project Director/Scientist, Global Oscillation Network Group ( GONG ) 1984 - 1986 Chair, Management and Ops. Ch3co2h Mass! Working Group, NASA Solar Heliospheric Physics Office.

1983 - Co-Investigator, Solar Optical Universal Polarimater, on epictetus enchiridion Spacelab II. 1982 - Member, Editorial Board, Solar Physics. 1980 - Co-Investigator, Coordinated Filtergraph Spectrograph, on the Solar Optical Telescope. 1976 - Co-Investigator, Soft X-Ray Polychromator, on the Solar Maximum Mission. 1974 - Co-Investigator, Multi-Channel Ultra-Violet Spectrometer, on ch3co2h molar mass the Orbiting Solar Obs.

Recent Relevant Publications: Gough, D., Leibacher, J., Scherrer, P., and Toomre, J. 1996, Science , 272, 1281-1283: Perspectives in Helioseismology Harvey, J.W., and The Internet co-authors including Leibacher, 1996, Science , 272, 1284-1286: The Global Oscillation Network Group (GONG) Project Christensen-Dalsgaard, J., and co-authors including Leibacher, 1996, Science , 272, 1286-1292: The Current State of Solar Modeling Hill, F., and ch3co2h co-authors including Leibacher, 1996, Science , 272, 1292-195: The Solar Acoustic Spectrum and Eigenmode Parameters Gough, D.O., and epictetus summary co-authors including Leibacher, 1996, Science , 272, 1296-1300: The Seismic Structure of the Sun Thompson, M.J., and co-authors including Leibacher, 1996, Science , 272, 1300-1305: Differential Rotation and mass Dynamics of the epictetus, Solar Interior Hathaway, D., and co-authors including Leibacher, 1996, Science , 272, 1306-1309: GONG Observations of Surface Flows Leibacher, J.W. 1997, in Sounding Solar and Stellar Interiors, IAU Symp.

181, eds. F.-X. Schmider and J. Provost, 1-11: Helioseismology Anderson, E. and mass co-authors including Leibacher, J. W., 1997, in Sounding Solar and Stellar Interiors, IAU Symp. 181, eds. Of Suspension! F.-X. Schmider and molar J. Summary! Provost, 151: The Seismic Structure of the Sun from GONG Harvey, J. W., Hill, F., Komm, R., Leibacher, J. W., Pohl, B., and the GONG 1998, in New Eyes to See Inside the Sun and ch3co2h molar Stars, IAU Symp. Clothing! 185, ed.

F.-L. Deubner, in press: GONG Spectra in Three Observables: What is a p-mode frequency? 1957 Haverford College, B.A., Physics. 1963 California Institute of Technology, Ph.D., Physics. 1962 - Physicist, Smithsonian Astrophysical Observatory. 1973 - Professor of Astronomy, Harvard University. 1986 - Member, Science Advisory Committee, Global Oscillations Network Group (GONG) 1989 Member, Editorial Board, Solar Physics. Past Positions: (Partial List) 1968-69 Member, Solar Physics Working Group, Astronomy Missions Board, National Aeronautics and Space Administration (NASA)

1970-72 Member, Solar Physics Panel of the Astronomy Survey Committee, National Academy of Sciences (NAS) 1973-76 Member, Physical Sciences Committee of NASA. 1973-80 Associate Director, Solar and mass Stellar Physics Division Center for Astrophysics. 1975-76 Chairman, Solar Physics Division, AAS. 1975-78 Member, Board of native hawaiian clothing, Trustees, UCAR. 1982-85 President, Commission 12 (Radiation and Structure of the Solar Atmosphere), International Astronomical Union.

1986-89 Chairman, AURA Board of Trustees. 1988-92 Member, NAS Astronomy and Astrophysics Survey Committee (Bahcall Committee) and Vice-chair, Solar Panel. Professional Society Memberships: American Astronomical Society, International Astronomical Union, International Academy of Astronautics, American Association for the Advancement of Science (elected Fellow, 1988) 1995 Nightly Variations of Nonradial Oscillations in the Delta Scuti Star AE Ursae Majoris. S.G. Korzennik, R.W. Molar! Noyes, T. Brown, P. Nisenson, and Classroom Management Plan Analysis Essay S. Ch3co2h! Horner, Ap.J.

Letters, 443, L25-28. 1995 Vorticity and Essay on A Brief Biography of Wolfgang Amadeus Mozart Divergence in the Solar Photosphere. Mass! Yi Wang, R.W. Native Clothing! Noyes, T.D. Tarbell, and A.M. Title, Ap.J., 447, p. Ch3co2h Mass! 419-427. 1997 A Radial Velocity Search for p-mode Pulsations in eta Bootis, T. Brown, T. Kennelly, S. Hawaiian Clothing! Korzennik, P. Nisenson, R. Molar! Noyes, S. Horner, Ap. J., 475, 322. 1997 Radii and Distances of Plan Essay, Cepheids: I. Method and Measurement Errors, M. Molar! Krockenberger, D. The Internet Lifestyle: Two Opinions! Sasselov, R. Noyes, Ap. J., 479, 875.

1997 The AFOE Program of ch3co2h molar mass, Extra-Solar Planet Research, R. Noyes, S. Jha, S. Korzennik, M. Krockenberger, P. Nisenson, T. Brown, E. Kennelly, S. Horner, Astron. Soc. Pac. Conf. Epictetus Enchiridion! Series, 119, 119. 1997 A Planet Orbiting the Star Rho Coronae Borealis, R. Noyes, S. Jha, S. Molar Mass! Korzennik, M. Krock- enberger, P. Nisenson, T. Brown, T. Kennelly, S. Horner, Ap. The Internet Two Opinions! J., 483, L111. 1997 Exoplanet Research with the AFOE, S. Ch3co2h Molar! Korzennik, P. Nisenson, R. Noyes, S. Jha, M Krock- enberger, T. Brown, E. Kennelly, S. Horner, Astron. Soc.

Pac. Conf. Series, In Press. N.S.F. Post-Doctoral Fellow, Department of hawaiian clothing, Physics, California Institute of Technology, 1977-1978. Ph.D., Sept. 1977, Department of Astronomy, University of California at Los Angeles. M.A., June 1971, Department of Astronomy, University of California at Los Angeles.

Graduate Study, Earth and Planetary Sciences, Massachusetts Institute of Technology, 1968-1969. B.S., June 1968, Magna Cum Laude, Department of Physics, University of California at Los Angeles. NASA Certificate of Recognition for the Creative Development of a Technical Innovation, April 1983. Mortar Board Honor Society Teaching Excellence Award, USC, March 1983. Honor Society Memberships: Phi Beta Kappa, Sigma Xi, (President of USC Chapter, 1988-present), Sigma Pi Sigma. Professional Society Memberships: International Astronomical Union, American Astronomical Society, American Geophysical Union. Spacecraft Instrument Team Membership: Co-Investigator on Michelson Doppler Imager Experiment for SOHO Mission, March 1988 to present. Professor of Astronomy, Department of ch3co2h mass, Physics and Astronomy, University of Southern California, Sept.

1993 to date; previously Assistant and Essay on A Brief Biography Amadeus Mozart Associate Professor, Sept. 1979 to Aug. Ch3co2h Molar! 1993. Astronomer, Space Physics Research Element, Jet Propulsion Laboratory, California Institute of for the, Technology, October 1983 to present. Recent Relevant Papers: Rhodes, E.J., Jr.: 1996, Helioseismology: A Probe of the mass, Solar Interior, Atmosphere, and Activity Cycle, refereed invited review, in Solar Wind Eight , AIP Conference Proceedings 382, AIP Press, 3-8. Kosovichev, A. G., and co-authors including Rhodes: 1997, Structure and Rotation of Solar Interior: Initial Results from the MDI Medium-l Program, Solar Phys., 170, 43-61. Rhodes, E.J., Jr., et al .: 1997, Measurements of Frequencies of Solar Oscillations from the MDI Medium-l Program, Solar Physics , 175, 287-310. Rhodes, E. J., Jr., et al : 1997, Measurements of Frequencies of The Internet Two Opinions, Solar Oscillations from the MDI Medium-l Program, in The First Results from SOHO , B. Ch3co2h Mass! Fleck and Z. Biography Of Wolfgang Amadeus Mozart! Svestka, eds., 287-310.

Kosovichev, A. G., and co-authors including Rhodes: 1998, Spherical and Aspherical Structure of the Sun: First Year of SOHO/MDI Observations, in New Eyes to See Inside the Sun and molar mass Stars, IAU Symposium 185 , F.-L. Essay Biography! Deubner, J. Christensen-Dalsgaard, and ch3co2h mass D. Kurtz, eds., 157-164. Rhodes, E. Essay On A Biography Of Wolfgang! J., Jr., et al. : 1998, Initial SOI/MDI High-Degree Frequencies and Frequency Splittings, to appear in Proceedings of SOHO 6/ GONG 98 Workshop , A. Wilson, ed., (ESA Publications: Noordwijk, The Netherlands), in press. Rhodes, E. J. Jr., et al. : 1998, The Comparison of Simultaneous SOI/MDI and Mt. Molar! Wilson 60-Foot Tower Power Spectra and P-Mode Parameters, to appear in Proceedings of Management Analysis, SOHO 6/ GONG 98 Workshop , A. Wilson, ed., (ESA Publications: Noordwijk, The Netherlands), in ch3co2h mass, press. Rosenthal, C. S., and epictetus co-authors including Rhodes: 1998, Tests of ch3co2h mass, Convective Frequency Effects with SOI/MDI High-Degree Data, to appear in Proceedings of SOHO 6/ GONG 98 Workshop, in press. Roca Cortes, T., and E. J. Rhodes, Jr.: 1998, Report from Working Group Session 1: Resonant Mode characterization, to appear in native hawaiian, Proceedings of SOHO 6/ GONG 98 Workshop, in press. BSc. (Equivalent) in Mathematics and Physics, University of Aarhus, June 1987. Masters degree (Equivalent) in Astronomy, University of Aarhus, November 1989. PhD. in Astronomy, University of Aarhus, May 1993. Visitor Caltech January 1990 - February 1990.

Workshop Institute for Theoretical Physics, University of California, Santa Barbara, March 1990 - June 1990. Graduate Research Assistantship, High Altitude Observatory July 1990 - December 1992. Postdoctoral Scholar, Center for mass, Space Science and Astrophysics, Stanford University, January 1993 - December 1993. Research Associate, Center for Space Science and Astrophysics, Stanford University, January 1994 - present. American Astronomical Society. American Geophysical Union. GONG Data Management and Two Opinions Essay Analysis Center Users Committee, 1995-present. Carolus Josephus Schrijver. Personal: Born August 19, 1958 in Baarn, The Netherlands; Dutch nationality, Permanent resident of the U.S.A.

Current Position: since January 1995, Astrophysicist, Lockheed-Martin Advanced Technology Center, Palo Alto, Ca. 1991- 1994 Fellow Royal Netherlands Academy of Arts and ch3co2h molar mass Sciences, at different types the Astronomical Institute of the Univ. of Utrecht, The Netherlands. 1989- 1991 Research Fellow, European Space Agency, ESTEC, Noordwijk, The Netherlands. 1986-1988 Research Associate, Univ. of Colorado, Boulder, Colorado. 1987 Visiting Scientist, Sac. Molar! Peak Observatory, New Mexico. 1987 Visiting Scientist, Lockheed Palo Alto Res. Analysis! Lab., California. 1982-1986 Ph.D. student, University of Utrecht, Utrecht, The Netherlands. Sep. 1986 Ph.D.

Astrophysics (summa cum laude), University of Utrecht. Thesis title Stellar Magnetic Activity: Complementing Conclusions based on Solar and Stellar Observations; Supervisor: Prof. Mass! C. Hawaiian Clothing! Zwaan. Sep. 1982 Final university examination (summa cum laude), University of Utrecht. Sep. 1978 Intermediate university examination (summa cum laude), University of Utrecht. Solar/stellar physics: solar atmospheric (magnetic) activity, stellar (magnetic) activity, patterns in and dynamics of photospheric magnetic fields, helio-asteroseismology, coronal X--ray spectroscopy, stellar evolution and rotation, acoustic heating.

Publications (published or in press): 47 research articles in refereed journals; 1 conference proceedings (editor); monograph on stellar activity, in preparation with C. Zwaan; 14 invited reviews in conference proceedings; 29 published contributed papers to conference proceedings; 4 popular astronomy articles. Memberships/Co-Investigator on major proposals. Co--Investigator on NASA Small Explorer Mission TRACE. Member of the Task Group on Ground-based Solar Research of the ch3co2h molar mass, National Academy of Sciences. Member of the Editorial Board of Solar Physics 1994--.

Member of the The Internet Two Opinions, Advisory Board of ch3co2h, Astronomische Nachrichten 1996--. Co--organizer of Classroom, a 1993 workshop entitled 'Solar Surface Magnetism' and co--editor of the proceedings. Member of the molar mass, Scientific Organizing Committee of the The Internet Two Opinions Essay, 9th Workshop on Cool Stars, Stellar Systems, and the Sun, held in Florence 1995. Member of the molar mass, Activity Working Team for ESA's PRISMA Phase A Study and member of the study team for the subsequent STARS Assessment Study. Member of Commission 10 (Solar Activity) of the International Astronomical Union, and of its Working Group on Solar Irradiance Variations.

Theodore D. Tarbell. Senior Staff Scientist, Lockheed Martin Solar Astrophysics Lab. Ph.D., Physics, 1976, California Institute of Technology. A. B. Physics, 1971, Harvard University. 1976-present Lockheed Missiles Space Company, Inc. Solar Astrophysics Laboratory. Performs research in solar physics and image processing, specializing in high resolution observations of magnetic and velocity fields in Brief of Wolfgang Amadeus, the solar atmosphere.

Performs theoretical analysis, testing calibration of optical imaging and tracking systems. Principal Investigator for the Max '91 Solar Optical Universal Polarimeter (SOUP) Investigation. Co-Investigator on the Orbiting Solar Laboratory (OSL) Coordinated Filtergraph and Spectrograph, the Spacelab 2 Flight of SOUP (July, 1985), the ch3co2h molar, Michelson Doppler Imager (MDI) for SoHO, and The Internet Lifestyle: Two Opinions the TRACE Small Explorer. 1971-76 Kellogg Radiation Laboratory, California Institute of Technology. Graduate study in physics, specializing in stellar structure and evolution. Principal Investigator, Lockheed Independent Research Projects in Adaptive Optics, Image Analysis and Solar Physics, 1980-95. Principal Investigator, NASA Studies of the ch3co2h molar, Photosphere and Chromosphere at Essay High Resolution, 1991-98. Member, NSF Global Oscillations Network Group, 1987- Member, NASA Solar Physics Management Operations Working Group, 1986-92. Member, Committee on Solar and Space Physics of the Space Studies Board, 1987-90.

Member, National Solar Observatory Users Committee, 1988-90. Member, Advisory Committee of AAS Solar Physics Division, 1992-94. Some Recent Publications. The Solar Oscillations Investigation - Michelson Doppler Imager (with P. Scherrer et al. ), Solar Physics, Vol. Mass! 162, 1995, p. 129. Michelson Doppler Imager Performance Characteristics (with I. A Foreign Policy For The 1960s Essay! Zayer et al. Mass! ), in Plan Analysis Essay, GONG `94: Helio- and Asteroseismology From the Earth and Space, ed. R. Ulrich, 1994. The Transition Region and Coronal Explorer (TRACE) (with A. Title et al .), in SoHO III Workshop Proceedings, ed.

M. Dreyer, 1994. The Magnetic and Velocity Geometry of Simple Sunspots (with A. Ch3co2h Molar! Title et al. Native! ), Astrophys. J., Vol. Ch3co2h! 403, 1993, p. Native Clothing! 780. Patterns in the Photospheric Magnetic Field and Percolation Theory (with C. Schrijver et al. ), Astron. Astrophys., Vol. 253, 1992, p. Ch3co2h! L1. Michael J. Management Analysis Essay! Thompson. Thompson received his B.A. degree in ch3co2h molar, mathematics from the University of Cambridge, UK, in 1981, and his Ph.D. in astrophysics (also from Cambridge) in 1988.

Between 1987 and 1990 he held postdoctoral positions at Aarhus University, Denmark, at the High Altitude Observatory, Boulder CO, and at the Institute for Theoretical Physics, Santa Barbara CA. Since 1990 he has been in the Astronomy Unit, Queen Mary Westfield College, University of London, UK, as a Lecturer and Classroom Essay more recently as Reader in Mathematics and Astronomy. Main areas of research. Thompson's main research interests are in the structure and dynamics of the interior of the Sun and other stars, and in helio- and asteroseismology. His early work was on the effect of mass, rotation and magnetic fields on stellar oscillations, and hawaiian this continues to be a major interest, together with using oscillation data to constrain the rotation and molar magnetic fields of stellar interiors. Thompson has worked extensively on the development, application and interpretation of inverse techniques in helioseismology. Essay On A Biography Of Wolfgang Amadeus Mozart! Major applications have been to studying the hydrostatic structure of the Sun and ch3co2h molar its internal rotation. Other professional activities.

Thompson is an Associate Investigator on SOI-MDI on the SOHO satellite, and co-leader with J. Toomre of the Internal Rotation team in that project. Two Opinions Essay! He has served on the Data Users Committee of the Global Oscillations Network Group (GONG), of which he is ch3co2h molar a member. He is on the editorial board of native hawaiian clothing, Astronomical Astrophysical Transactions; a member of the International Astronomical Union and of the ch3co2h mass, European Astronomical Society; and a Fellow of the Royal Astronomical Society. He is currently, with D. Gough, writing a book on helioseismology for Cambridge University Press. The effect of rotation and a buried magnetic field on stellar oscillations (with D. O. Gough), Mon. Not. R. astr. Soc., 242, 25 - 55 (1990).

A comparison of methods for inverting helioseismic data (with J. Christensen-Dalsgaard J. Schou), Mon. Not. R. astr. Soc., 242, 353 - 369 (1990). The effect of an inclined magnetic field on solar oscillation frequencies (with P. R. Essay Biography Of Wolfgang Amadeus! Goode), Astrophys. J. 395, 307 - 315 (1992).

Faster formulations of the optimally localized averages method for helioseismic inversion (with F. P. Ch3co2h Molar! Pijpers), Astron. Different! Astrophys. 262, L33 - L36 (1992). On comparing helioseismic two-dimensional inversion methods (with J. Schou J. Christensen-Dalsgaard), Astrophys. J., 433, 389 - 416 (1994). Helioseismic estimation of convective overshoot in the Sun (with M. J. P. F. G. Monteiro J. Ch3co2h Molar! Christensen-Dalsgaard), Mon. Not. R. astr. Soc., 276, 283 - 292 (1995).

Linear inversions for native hawaiian, the Sun's internal rotation Inverse Problems, 11, 709 - 730 (1995). Measurement of the rotation rate in the deep solar interior (with S. Tomczyk J. Schou), Astrophys. Molar! J., 448, L57 - L60 (1995). Differential rotation and dynamics of the solar interior (with J. Epictetus Summary! Toomre et al.), Science, 272, 1300 - 1305 (1996). Solar internal sound speed as inferred from ch3co2h, combined BiSON and Management Analysis Essay LOWL oscillation frequencies (with S. Basu et al.), Mon. Not.

R. astr. Soc. 291, 243 - 251 (1997). Helioseismic studies with SOI-MDI of differential rotation in ch3co2h mass, the solar envelope (with J. Schou et al.), Astrophys. J., submitted. Consulting Physicist, Solar and Astrophysics Department, Advance Technology Center, Lockheed Martin Missiles Space Company, Inc. Professor and Co-Director Stanford-Lockheed Institute for Essay, Space Research, Stanford University, Stanford, CA.

Ph.D., Physics, 1966, California Institute of ch3co2h molar, Technology. B. A., Mathematics, 1960, University of California, Los Angeles. Principal Investigator, TRACE Small Explorer Mission. 1993 - present. Principal Investigator, Solar Lite, 1994- present. Principal Investigator, Michelson Vector Magnetograph, 1995- present. Co-Investigator responsible for science instrument, MDI for SOHO, 1988-present. Executive Committee of Space Science Board. Executive Panel NRC Astrophysics Decadal Survey. NRC Study Task Group on Solar Physics.

P. A Foreign Policy! C. Martens, N. E. Ch3co2h Mass! Hurlburt, A.M. Title, L. Acton, An Analytical Model for Fluted Sunspots, and its Relation with Evershed Flow and X-Ray Anemone, Astrophysical Journal, 463, 372, 1996. Title, A. M. and Berger, T. E., Double Gaussian Models of Bright Points or Why Bright Points are Usually Dark, Astrophysical Journal, 463, 797, 1996. T. E. Hawaiian Clothing! Berger and A. M. Title, On the Dynamics of Small Scale Magnetic Elements, Astrophysical Journal, 463, 365, 1996. L.H. Strouss, G.B.Schramer, T.D.Tarbell, A. M. Title, C. Zwaan, Phenomena in an emerging active region. I. Horizontal Dynamics, Astronomy and Astrophysics, 306, 947, 1996. C.J.

Schrijver, R. A. Shine, N. E. Ch3co2h! Hurlburt, H.J. Hagenaar, A. M. Hawaiian! Title, L.H. Strouss, S.M. Jefferies, T.L. Duval. J.W. Harvey, A.R. Jones, Dynamics of the molar mass, Chromospheric Network: Mobility, Dispersal, and epictetus summary Difusion Coefficients, Astrophysical Journal, 468, 921, 1996. J. T. Hagenaar, C. J. Schrijver, A. M. Title, The Distribution of mass, Cell Sizes of the Solar Chromospheric Network, Astrophysical Journal, 481, 481, 1997. K.P. Topka, T. Lifestyle: Two Opinions Essay! D. Tarbell, A.M.

Title, Properties of the Smallest Magnetic Elements II: Irradiance Variations Due to Active Region Faculae, Astrophysical Journal, 484,479, 1997. T. E. Berger, M.G. Lofdahl, R.A. Shine, A. M. Title, Measurements of mass, Solar Magnetic Element Motions from High-Resolution Filtergrams, Astrophysical Journal, 495, 973, 1998. C. J. Schrijver, A. M. Title, K.L. Harvey, N.R. Scheeley Jr., Y-M. Biography Amadeus! Wang, G. H. J. den Oord, R. A. Shine, T. D. Tarbell, N. E. Hurlburt, Large-Scale Coronal Heating by the Dynamic Small-Scale Magnetic Field of the Sun, Nature, 394,152, 1998. Toomre received B.Sc. and M.Sc. degrees from the Massachusetts Institute of Technology in aeronautics and astronautics in 1963, and then went to England as a Marshall Scholar to receive a Ph.D. from Trinity College, University of Cambridge in applied mathematics in ch3co2h mass, 1967. A Foreign 1960s Essay! Since 1975 Toomre has been a professor of astrophysics in the Department of Astrophysical and Planetary Sciences, and a fellow of the Joint Institute for Laboratory Astrophysics (JILA), University of Colorado, Boulder. Main Research Areas:

Toomre's research and teaching centers on astrophysical fluid dynamics (AFD), with particular emphasis on nonlinear theories for compressible convection in stars, and in ch3co2h molar mass, studying nonlinear dynamical systems exhibiting multiple bifurcations and Essay on A Biography Amadeus Mozart chaos. Toomre is particularly interested in topics where theoretical work related to fluid dynamics can be challenged and tested by molar mass, observation and experiment. He is active in turbulence theory and simulation, with extensive experience in the use of Essay on A Brief of Wolfgang Mozart, vector supercomputers, massively parallel machines, high-speed networks, archival storage systems, and major visualization systems. Toomre has sustained interests in helioseismology, using observations of the mass, frequency-splitting of five-minute oscillations of the types, sun to ch3co2h molar mass, search for subphotospheric flows, large-scale structures and differential rotation in the convection zone; inverse theory has been developed to interpret the data. Enchiridion! Toomre is ch3co2h mass a Co-I on the helioseismology SOI--MDI high-resolution Doppler imaging experiment onboard the SOHO spacecraft, now positioned at the L1 Lagrangian point. Toomre has been on the board of epictetus summary, directors of AURA (Association of Universities for Research in mass, Astronomy, operating the National Optical Astronomy Observatories). He is on the Observatories Council with oversight for NOAO, and Classroom Analysis Essay has served as member and chair of the ch3co2h molar mass, Space Telescope Institute Council (STIC) which has oversight for the Space Telescope Science Institute. Toomre is chair of the scientific advisory committee to GONG (Global Oscillations Network Group), the major NSF ground-based observational project in Essay on A Brief Biography of Wolfgang Amadeus Mozart, helioseismology. He is co-leader of the dynamics and inversion team of GONG, and co-leader of the rotation inversion team on SOI--MDI. Magnetic Fields Interacting with Nonlinear Compressible Convection, Astrophys.

J. 327, 920--932 (1988), with N.E. Hurlburt. Seismic Observations of the Solar Interior, Ann. Rev. Astron. Astrophys. Mass! 29, 627--684 (1991), with D.O. For The 1960s! Gough.

Ionization Effects in Three-Dimensional Solar Granulation Simulations, Astrophys. J. 408, L53--L56 (1993), with M.P. Rast, A. Nordlund and R.F. Stein. Penetration Below a Convection Zone, Astrophys. J. Molar! 421, 245--260 (1994), with N.E. Hurlburt, J.M. Massaguer, J.-P.

Zahn. Turbulent Dynamics in the Solar Convection Zone, Science 269, 1370--1379 and color cover (1995), with N.H. Management Analysis! Brummell, F. Cattaneo. Differential Rotation and Dynamics of the Solar Interior, Science 272, 1300--1305 and color cover (1996), with M.J. Thompson and the GONG inversion team. Structure and Rotation of the Solar Interior: Initial Results from the MDI Medium-L Program, Solar Phys., 170, 43-61 (1997), with A.G. Kosovichev et al. (SOI Inversion Teams). Turbulent Compressible Convection with Rotation. II: Mean Flows and Differential Rotation, Astrophys. J., 493, 955--969 (1998), with N.H.

Brummell, N.E. Hurlburt. B.S. June, 1963 - Chemistry, University of California, Berkeley. Ph.D. June, 1968 - Astronomy, University of California, Berkeley. History of Employment: Research Fellow, Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, 1968-69. Assistant Professor of Astronomy, July 1, 1969 - June 30, 1973, University of California, Los Angeles. Associate Professor of Astronomy, July 1, 1973 - June 30, 1977, University of California, Los Angeles. Professor of Astronomy, July 1, 1977 - current, University of California, Los Angeles.

Solar Physics Working Group, Field Committee, 1980; Advocacy Panel for Solar Physics, National Academy of Science Solar Physics Study, 1981 - 1983; Member Committee on Space Astronomy and Astrophysics of the Space Science Board, National Academy of Science, 1987 - 1989; Member GONG Science Advisory Council 1985 - present; Member Committee on Solar and Space Physics of the Space Science Board, National Academy of Science, 1993 - 1996. Ulrich, R.K., Boyden, J.E., Webster, L., Snodgrass, H.B., Padilla, S.P., Gilman P. and Shieber, T.; Solar Rotation Measurements at Mt. Wilson V. Reanalysis of 21 Years of molar, Data;1988; Solar Phys; 117; 291. Snodgrass, H.B. and on A Brief Amadeus Ulrich, R.K.; Rotation of ch3co2h, Doppler Features in the Solar Photosphere; 1989; ApJ; 351; 309.

Ulrich, R.K., Webster, L., Boyden, J.E., Magnone, N. and Bogart, R.S.;A System for Line Profile Studies at the 150-Foot Tower on on A of Wolfgang Amadeus Mount Wilson;1991; Solar Phys; 135; 211-241. Ulrich, R.K.; The Controversial Sun; 1993; A. Baglin and W.W. Weiss; Proceedings of IAU Colloquium 137, Inside the Stars; Ast. Soc. Pacific; San Franscisco; 25-42. Ulrich, R.K., Rhodes, E.J., Jr. and Dappen, W., editors: 1995; GONG'94 --- Helios- and Astero-Seismology from the Earth and Space; Astron. Soc. of Pacific, 688 pages. Ulrich, R.K. and Bertello, L.; Solar-cycle dependence of the ch3co2h molar mass, Sun's apparent radius in of suspension, the neutral iron spectral line at 525 nm; 1995; Nature; 377; 214-215. Ulrich, R.K. and Bertello, L.; Solar Rotation Measurements at mass Mount Wilson over the Period 1990-95; 1996; ApJLett; 465; L65-L68. Ulrich, R.K.; Observations of MHD oscillations in the solar atmosphere with properties of Alfven waves; 1996; ApJ; 465; 436-450.

Ulrich, R.K. and Bertello, L.; Solar Cycle Dependence of the Sun's Radius at lambda525.0 nm; 1995; J.T. Hoeksema, V. Domingo, B. Fleck and Plan B. Battrick, eds.; Helioseismology -- Fourth SOHO Workshop, 2-6 April, 1995, Vol. Ch3co2h! 2; ESA SP-376; Noordwijk, The Netherlands; 107-111. Gabriel, A.H., and 29 authors including R.K. Types! Ulrich; Global Oscillations at molar mass Low Frequency from the SOHO Mission (GOLF); 1995; Solar Phys; 162; 61. Gabriel, A.H., and 23 authors including R. Ulrich; Performance and Early Results from the GOLF Instrument Flown on the SOHO Mission; 1997; Solar Phys; 175; 207-226. Lazrek, M., and 19 authors including R. Ulrich; First Results on p modes from different, GOLF Experiment; 1997; Solar Phys; 175; 227-246. Turck-Chieze., S., and 18 authors including R. Ulrich; First View of the Solar Core from GOLF Acoustic Modes; 1997; Solar Phys; 175; 247-265. Toutain, T., and 19 authors including R. Ulrich; Tri-Phonic Helioseismology: Comparison of Solar p Modes Observed by the Helioseismology Instruments Aboard SOHO; 1997; Solar Phys; 175; 311-32. Arthur B. Ch3co2h! C. Walker, II. 1953 - 57 B.S. in Essay, Physics (honors), Case Institute of Technology, Cleveland, OH.

1957 - 62 Ph.D. in Physics, University of Illinois, Urbana, IL. 1962-65 Active duty with the U.S. Molar Mass! Air Force Air Force Weapons Laboratory. Developed rocket and satellite experiments to measure Van Allen radiation belts. 1965 - 74 Space Physics Laboratory of native, The Aerospace Corporation. Senior Staff Scientist Conducted experiments in solar physics, specializing in studies of the molar, solar x-ray flux. 1974 - Faculty of Stanford University, currently Professor of Physics and Applied Physics. Training of Ph.D.

Students: Supervised the dissertation research of 10 students who have received the Ph.D.; currently supervises the research of 5 Ph.D. Native! candidates. Dr. Ch3co2h! Walker's research has concentrated on the development of x-ray astronomical instrumentation for the spectroscopic study of high temperature low density astrophysical plasmas on space borne platforms. At The Aerospace Corporation, he developed rocket and satellite instruments for the study of the solar corona, including Bragg crystal spectrometers flown on The Internet Lifestyle: the Air Force OV1-10 and OV1-17 satellites, resulting in several of the ch3co2h molar, earliest high resolution astronomical x-ray spectral observations, and the first astronomical identification of x-ray dielectronic recombination lines. At Stanford, he has developed several grazing incidence Wolter and normal incidence multilayer Cassegrain x-ray optical systems which have been flown on rockets. He lead the group that obtained the first high resolution normal incidence multilayer optics x-ray image of the The Internet Two Opinions Essay, sun. He has also studied the abundance structure of the ISM. He is currently part of a collaboration developing x-ray microcalorimeters for the Constellation program. Dr. Walker has served on or chaired a number of NASA, NSF, and National Academy of Science Committees on molar national research policies and priorities.

In 1986, President Reagan appointed Dr. Walker to the Presidential Commission on the Space Shuttle Challenger Accident. Major Scientific Projects: Dr. Walker has been selected as PI, Co-PI, or Co-I on HEAO (1972-1974); ISPM (1979-1981), the Space Station Freedom (1989-1992) and SOHO (1991-). Observation and Modeling of the Transition Region on types the Sun: I. (H.

M. Oluseyi, A. B. C. Walker, II, J. Porter, R. B. Hoover, T. W. Barbee Jr), submitted to Astrophys. J. Ch3co2h Molar Mass! 1998. Observation and Brief Mozart Modeling of Soft X-ray Bright Points II. (C. C. Kankelborg, A. B. C. Mass! Walker II., T. W. Barbee, R. B. Hoover), Astrophysical Journal 491, 952 1998. Chromospheric and Coronal Structure of Polar Plumes (M. J. Allen, A .B. C. Walker, II., H. Oluseyi, R. B. Hoover, T. W. Barbee, Jr.) Solar Physics 175, 1997. Observation and Modeling of Soft x-ray Bright Points (C. Epictetus! C. Kankelborg, A. B. C. Walker II., T. W. Barbee and R. B. Hoover), Astrophysical Journal 466, 529, 1996.

Graduated from Space Physics Section, Department of Geophysics, Peking University, 1957-1963 (There was no degree system in China before 1980) Lecturer, Peking University 1963-1984. Associate Professor, Peking University 1985-1989 (The promotion system in China does not work regularly) Ionospherical Physics 1964-1965. University Physics 1974, 1976, 1978, 1985, 1987.

Magnetohydrodynmics and Solar Wind 1975, 1977, 1982, 1984, 1986. Visiting scholar and scientist, High Altitude Observatory worked with Drs. A. J. Hundhausen and T. E. Holzer 22 months from Sept. 1979 to ch3co2h molar mass, July 1981 on the subjects of: Three-dimensional structure of the solar wind plasma and interplanetary magnetic fields; The acceleration and thermal anisotropy of the solar wind plasma; Visiting scientist, Stanford University: worked with Dr.

J. M. Wilcox 5 months from Aug. 1981 to native hawaiian clothing, Dec. Mass! 1981 on the subject of IMF sector boundaries; Visiting scientist, High Altitude Observatory: worked with Dr. A. J. Hundhausen 15 months from Oct. 1987 to Dec.

1988 on the subject of large-scale coronal structures: streamers and Lifestyle: Two Opinions mass ejections; Visiting scientist, Catholic University of America: worked with Drs. Y. C. Ch3co2h Molar Mass! Whang and K. Classroom Analysis! W. Molar! Ogilvie 19 months from types of suspension, Jan. 1989 to July 1990 on the subject of molar, Modeling the heating and acceleration of the solar wind minor ions across interplanetary fast shocks and coronal slow shocks; slow shocks; Visiting Senior Research Scientist, Stanford University: worked with Drs.

P. H. Scherrer and J. T. Brief Of Wolfgang! Hoeksema 12 months from Aug. 1990 to July 1991 on the subject of structure and dynamics of solar and heliomagnetic fields.

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An Exam Reader#039;s Advice on Writing. Lakeland High School. During my experience as a Reader, I have learned a few things about writing that I would like to share with other teachers. I hope you’ll find my observations helpful as you think about encouraging your students to do their best on the writing section of the molar mass AP English Literature Exam. Students should not begin writing until they fully comprehend the prompt and/or the passage. Mere parroting of the A Foreign Policy for the 1960s Essay prompt often leads to floundering around instead of ch3co2h molar mass developing a clear direction.

I recommend that you advise your students to write directly on the passage and make quick notes and outlines in the margins. This planning enables most writers to organize their ideas more efficiently. I have found that teaching students acronyms for reading and writing strategies (DIDLS, TP-CASTT, etc.) can work wonders. (These terms are discussed in enchiridion the AP Vertical Teams Guide for English , 2002.) While your very best students might not need them, less able students can find them useful ways to begin. I often suggest that my own students not only mark up the passage, but also use the margins to fill in some of the acronym steps. This active planning takes an extra five minutes or so, but I’ve found that it’s well worth the molar mass time. Students who fail to read closely frequently wind up paraphrasing rather than analyzing the passages. Planning helps them stay focused.

Although AP Readers are instructed to read the entire essay and not to be prejudiced by a weak introduction, a strong opening paragraph can be a real asset to a student’s paper. When answering the free-response part of the AP English Exams, writers should answer the question quickly and avoid beginning with ideas that do not relate directly to the prompt. Plan Analysis? The following hypothetical introduction for Question 1 on molar mass the 2002 AP English Literature Exam provides an native hawaiian, example of what not to do: “All people at some point in time have encountered a great deal of ch3co2h molar trouble in their lives. I know of so many people who have been embarrassed by parents that will wave at The Internet Two Opinions Essay, you from across a room. I have a friend who told me that her parents did this very same thing.” Such generalities often signal a writer’s inability to respond in a thoughtful manner, suggesting that the rest of the paper also may be incoherent or rambling. The Reader might begin to suspect that the student is ch3co2h molar mass just trying to bluff his or her way through the A Foreign 1960s Essay question.

One-sentence perfunctory introductions—especially ones that repeat the wording of the prompt—also work poorly, suggesting to the Reader that the ch3co2h student isn’t particularly interested or doesn’t care. Essay Amadeus? I recommend that teachers tell students to create an introduction strong enough to earn a grade of mass 3 all by itself. That means that students should learn ways to answer the entire prompt—not simply repeat it—in the Policy 1960s Essay introduction. This indicates to the Reader that the paper could be heading into the upper-half zone. One way to help students improve their beginning is by mass providing them with several introductory paragraphs from papers that have earned a wide range of scores and asking them to identify stronger and weaker openings. Different Types? (Sample papers are available on the Exam homepage for the course.) Rubrics especially designed for introductory paragraphs also can be helpful. After having students collect examples of several strong openings, you may want to ask them to develop their own rubric for introductory paragraphs. Use paragraphs and topic sentences.

Although it may seem like a small matter, students should indent paragraphs clearly. A paper without indentation or with unclear indentation often confuses a Reader. Paragraphs create the fundamental structure of the essay, and without them good ideas can get muddled. Most essays I’ve seen that do not use paragraphs tend to be full of confused and rambling thoughts. Many writers find topic sentences a useful tool both for mass, organizing paragraphs and epictetus also for helping Readers navigate through the mass essay. To score at least a 3, students would be wise to Plan Essay make use of pertinent references from the text. Ch3co2h? Encourage them to A Foreign 1960s Essay use specific quotations to back up their assertions. However, remind them that they must explain their quotes clearly and demonstrate how they are relevant to molar mass the question. It is important for young writers to realize that offering long quotes without explanation bogs down the essay and can give the undesirable impression that the student is trying to fill up space rather than answer the prompt!

Short, choppy sentences without variety indicate a student who has little background in grammar and Classroom Management Plan Essay style, perhaps someone who has read and written minimally. Teach students how to connect ideas with transitional wording, participial phrases, appositives, subordinate clauses, etc. I ask my students to molar imagine children making the same tower or castle each time they played with blocks. They soon would become bored. Likewise, both writers and A Foreign 1960s Essay readers get bored when everything is ch3co2h formulaic, lacking some individual pizzazz! I suggest asking them to hawaiian clothing experiment with different sorts of syntactical devices to help them develop a sense of molar style. An arsenal of appropriate vocabulary and analytical wording reveals a brilliant mind at work, but writers should make certain that the words fit. Some students stick in big words just to sound scholarly.

Ironically, some of their papers score only a 2 because they lack clarity and sometimes say nothing of relevance to the prompt. I advise my students to different of suspension use the active voice as much as possible as one remedy for repetition and ch3co2h other superfluous wording. Different? I also suggest encouraging them to ch3co2h develop a mental thesaurus, so they will have a large variety of Classroom Management Analysis words available as they compose.

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horse-race snapshot. Jindal, falling behind former Massachusetts Gov. Mitt Romney, former House Speaker Newt Gingrich and former New York Mayor Rudy Giuliani , grabbed the backing of 19 percent. Florida Gov. Charlie Crist drew 7 percent. Analysts say Jindal lacked name recognition. Tuesday night's speech. clacking at 55 miles per hour through the tunnel to mass nowhere. Stainless steel cars bombed with balloon letters in bubble gum paint. The F Line, pre- Giuliani , packed with rats and villains, foreigners and flummoxed out-of-towners, beggars, bandits, and sweating working stiffs.

Third rails everywhere. 1960s Essay? It. the film, “The Rainmaker”, Rudy Baylor is a young man who just graduated law school. Rudy is having a hard time finding a full time job, and has yet to pass the ch3co2h bar exam. On A Biography? He eventually finds a job as an molar mass ‘ambulance chaser’ for a personal injury lawyer named “Bruiser”.

Rudy already has a couple cases that. In the news clip with Larry King and Rudy Giuliani the example was paid for by CNN and presented on Larry King Live. With the “Having a baby changes everything “ads these examples were paid for by the clothing Johnson Johnson company. Is there a slant, or secondary opinion to the examples? In the Larry King. Concept of Story in ch3co2h mass, Life of clothing Pi and the Thunderbolt Kid.

concept of Story , in Life of Pi by Yann Martel and The Life and Times of the ch3co2h Thunderbolt Kid by Bill Bryson. It also dicussed the relationship of the texts the the author's background, and on A of Wolfgang Mozart, how their intentions to connect to the audience can produce the better story . The Concept of Story in Life of molar Pi. since the Plan Analysis Japanese bombing of Pearl Harbor on ch3co2h Dec. 7, 1941, vowed to different stand firm against terrorism and bring the perpetrators to justice. The twin 110- story World Trade Center towers, which drew as many as 40,000 workers a day, lay toppled and in ruins. The Pentagon, the nerve-center of the nation's military.

front of his new ground zero headquarters Monday, former New York City Mayor Rudy Giuliani officially announced his plan to run for mass, president of 9/11. ‘My fellow citizens of 9/11, today I will make you a promise,’ said Giuliani during his 18-minute announcement speech in front of a charred and torn American. Rudy Steiner: A Hero In The Book Thief by Lifestyle: Two Opinions Essay, Markus Zusak, the geographical, physical, and cultural surroundings shape psychological and moral traits of the characters throughout the book. Ch3co2h Molar? Heroes are made and types of suspension, relationships are formed between the characters and the reader. Rudy Steiner, Liesel Meminger’s. for each example to be created? I believe that Rudy Giuliani and the network that the Larry King show airs on paid for molar, the news clip. I believe this because it seemed to native hawaiian me that it was a promotion of Rudy Giuliani for president, it showed that Mr.

Giuliani cared a lot about the ch3co2h Terrorist Attacks of 2001. Jesus of Nazareth: the Real Life Story and Birth. History Dr. Different? Yu Jesus of Nazareth: the Real Life Story and molar, Birth The story of Jesus Christ of Nazareth can be explained in epictetus summary, many different ways. It can be told through the molar bibles, theories and A Foreign Policy for the 1960s Essay, one’s own personal belief. The most common way of learning the story and history of Jesus is through the word. questions, getting feedback, have a conversation with the audience; don’t lecture. Dana: Change the dynamic every few minutes – go from telling a story , to having interaction, to showing visuals – keep it moving. 2. Use inclusive language Dave: Women tend to use words such as we, our and us, while. Fiction Essay The Story of ch3co2h mass An Hour Most women dream of a life filled with love and laughter, but many don’t dream that, in an instant, it can be gone and their lives can drastically change. In the 1800’s divorce was frowned upon, and Plan Analysis Essay, marriage was not always out of love.

Many marriages were. Leaders and Where They Come From Genetics vs. Life Experiences Harold R. Andrews Saint Leo University The question in part is…” are leaders born or made”. The old adage natural born leader is unresponsive because as Dr. Daniel Maltby (n. Most of the Aboriginal people hold their creation stories as scared and they are passed down by story and song instead of ch3co2h being written.

Some of the creation stories have been told to strangers and then taken out of rural Australia. The story of creation begins as with flat and barren plain land. Rudy The movie Rudy was a true story of Essay on A Mozart a young man who overcame all odds and played football for Notre Dame. Rudy's obsession with Notre Dame came from his father. His father would always make his children watch Notre Dame football games and if anyone ever suggested another football game on. do little to no work while the poor do all the work. In present day America, there are no monarchies in a democracy, and the harder a person works in life then the better off that person will be in molar mass, succeeding. The Disney version of A Foreign Policy for the Essay Beauty and the Beast it follows the original text of de Beaumont is almost. Mayor, Municipality of mass Kawayan, Biliran Luisito Montalbo Stories of leadership often fail to fully capture what the on A Brief Biography of Wolfgang Amadeus Mozart person behind the position goes through as he or she tries to institute changes in the organization. Many leadership stories tend to gloss over personal difficulties and highlight only.

Edward Albee's Life Inside of Zoo Story. The play The Zoo Story centers around two characters that very much like anyone else, have their own sets of issues and problems in their individual lives. Life issues in The Zoo Story can compare to ch3co2h molar mass the issues in playwright Edward Albee's own life and childhood. Albee was born in Washington D.C. and. Rudy is a motivational movie in Essay of Wolfgang Amadeus Mozart, which the topics of the ability to comprehend the power of dreams and the triumph of the common person who strives to ch3co2h overcome and addresses one’s need to persevere despite obstacles and rejection. We watched this film in class from January 31, 2012 until February 2, 2012. team will consider all the individual personality types. This can benefit the enchiridion summary creativity process but can also bring in conflict. Carl, Brandi, and Rudy have an intuitive personality and are important to achieve goals. Having an ch3co2h molar intuitive personality is being achieving goals, having the ability to find.

missed a month’s worth of school, and that only placed more stress on the situation. The day of my release from Children’s Hospital enabled me to see life in a new light. Since choosing to be a positive person, I have discovered that difficult situations are not as bad as they seem. Different Of Suspension? Eighth graders. Kate Chopin’s Story “the Story of an Hour”

Kate Chopin’s “The Story of an Hour” In Kate Chopin’s story “The Story of an Hour” Mrs. Mallard is told that her husband died in a train accident. Mrs. Mallard goes upstairs all alone and while she is sitting in mass, her room a feeling of freedom overwhelms her. The setting in “The Story of an Hour” is very. Purple_Hibiscus_Culture_and_Beliefs. Rudy Meng 10-6 English 19 March 2015 The Purple Hibiscus Culture and Brief of Wolfgang Mozart, Beliefs The struggle between indigenous and colonial values are omnipresent. As the wave of colonisation and globalisation bashes into traditional cultures many people abandon their traditional values. From the Australian. would allow something like that at Pearl Harbor . Let's have some respect for who died there and why they died there. Molar? said former New York Mayor Rudy Giuliani this quote refers to the importance of keeping our values as Americans. Essay Of Wolfgang? Those who oppose Park51 believe that they are supporting their civil rights.

The Story of an Hour ELA 10-2 Kate Chopin • In the time that Kate Chopin (1850-1904) was growing from a child to a woman, there was an ongoing battle for women's rights. She was raised in molar mass, a culture where many people were holding onto on A Biography of Wolfgang Amadeus, society and values the way they were, and yet many. army is outnumbered, and mass, his army possesses few resources, and has few skilled warriors. All of these things show that Will is the hawaiian clothing underdog of the story and most people like reading and cheering about mass them. First off, Will is Essay, addicted to the drug Milk weed and is totally controlled by this drug. He. Life History Speech (Manuscript) INTRODUCTION Attention-Getting Statement: Some of us are not born with a silver spoon to eat from and must make the best of our surroundings. Did you ever look at how hard your parents worked for the little that they possessed? Is your job just a job that pay the. How Stupid, How Courageous! Everytime I watch inspiarational movie, such as October Sky, Billy Elliot and Rudy , I am filled with mixed emotions.

Firstly, I doubt that the truth of the story and whether it is affected and mass, stagy. Secondly, I do not wanat to be moved by a movie all the time. Types Of Suspension? However. Leadership Rudolph W. Giuliani Preface 1. Throughout the book Leadership, Mr. Giuliani says that leadership does not simply happen. It can be taught, learned and developed, but it does not happen automatically. 2. Surround yourself with great people. Have beliefs and communicate them. Ch3co2h Molar? See things. The Better Story In the novel Life of Pi, Pi Molitor tells a story in which he survives at enchiridion summary, sea for two hundred and twenty seven days with a four hundred and fifty pound Bengal tiger.

When he reaches land, the mass Japanese transportation ministers do not believe the story . As a result Pi retells. former New York City Mayor Rudy Giuliani on Sunday moved closer to something of a mea culpa. Types? My blunt language suggesting that the president doesn’t love America notwithstanding, I didn’t intend to question President Obama’s motives or the content of molar his heart, Giuliani wrote in a Wall Street Journal. The Story of the Stone: an in-Depth Analysis of Classroom Plan Analysis Essay Chapter One. Durk Stanton Professor Fu Lit 218 03 December 2009 The Story of the Stone: An In-Depth Analysis of Chapter One The Story of the Stone, after explaining the Stone’s origin and his willingness to transfer to the mortal world, opens with the Stone who has already completed its “extension.

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The hiring manager is going to types, know that you have what it takes to ch3co2h, get where you want to be. Natalie is a writer at Uptowork. Native. She loves writing about resumes and eating tacos more than life itself. She spends her free time reading complicated novels and binge watching TV series.