The HMI science team includes those at the lead institutions (Stanford University, Lockheed-Martin Solar and

Astrophysics Laboratory, and the High Altitude Observatory) as well as Co-Investigators and Associated

Investigators at several other institutions.

HMI Science Team - Lead Teams
Name	Role	Institution	Phase B,C,D	Phase-E
HMI Lead Institutions
Philip H. Scherrer	PI	Stanford University	HMI Investigation	Solar Science
John G. Beck	A-I	Stanford University	E/PO Science Liaison	Surface Flows
Richard S. Bogart	Co-I	Stanford University	Data Pipeline and Access	Near Surface Flows
Rock I. Bush	Co-I	Stanford University	Program Manager	Irradiance and Shape
Thomas L. Duvall, Jr.	Co-I	NASA Goddard Space Flight Center	Time-Distance Code	Helioseismology
J. Todd Hoeksema	Co-I	Stanford University	Magnetic Fields	Magnetic Fields
Alexander G. Kosovichev	Co-I	Stanford University	Inversion Code	Helioseismology
Yang Liu	A-I	Stanford University	Vector Field Observable Code	Active Region Fields
Jesper Schou	Co-I	Stanford University	Instrument Scientist	Helioseismology
Xue Pu Zhao	Co-I	Stanford University	Coronal Code	Coronal Field Models
Alan M. Title	Co-I	LMSAL	HMI Instrument	Solar Science
Thomas Berger	A-I	LMSAL	* Vector Field Calibration	Active Region Science
Carolus J. Schrijver	Co-I	LMSAL	* Magnetic Field Assimilation Models	Active Region Science
Theodore D. Tarbell	Co-I	LMSAL	HMI Calibration	Active Region Science
Bruce W. Lites	A-I	High Altitude Observatory	Vector Field Inversions	Active Region Science
Steven Tomczyk	Co-I	High Altitude Observatory	Vector Field Inversions	Active Region Science
* Phase D only

HMI Science Team - US Co-Is
Name	Role	Institution	Phase B,C,D	Phase-E
HMI US Co-Investigator Institutions
Sarbani Basu	Co-I	Yale University	Ring Analysis Code	Helioseismology
Douglas C. Braun	Co I	NorthWest Research Associates	Farside Imaging Code	Helioseismology
Philip R. Goode	Co-I	NJIT, Big Bear Solar Observatory	Magnetic and Helioseismic Code	Fields and Helioseismology
Frank Hill	Co-I	National Solar Observatory	Ring Analysis Code	Helioseismology
Rachel Howe	Co-I	National Solar Observatory	Internal Rotation Inversion Code	Helioseismology
Sylvain G. Korzennik	Co-I	Smithsonian Astrophysical Obs.		Helioseismology
Jeffrey R. Kuhn	Co-I	University of Hawaii	Limb and Irradiance Code	Irradiance and Shape
H.D. Leka	Co-I	NorthWest Research Associates	Vector Field Calibration	Active Region Science
Charles A. Lindsey	Co-I	NorthWest Research Associates	Farside Imaging Code	Helioseismology
Jon A. Linker	Co-I	Science Applications Intnl. Corp.	Coronal MHD Model Code	Coronal Physics
N. Nicolas Mansour	Co-I	NASA Ames Research Center	Convection Zone MHD Model Code	Convection Physics
Thomas R. Metcalf ^*	Co-I	Colorado Research Associates	Vector Field Calibration	Active Region Science
Judit M. Pap	Co-I	University of Maryland	PICARD coordinator	Irradiance
Edward J. Rhodes, Jr.	Co-I	University of Southern California	Helioseismic Analysis Code	Helioseismology
Juri Toomre	Co-I	JILA, Univ. of Colorado	Sub-Surface-Weather Code	Helioseismology
Roger K. Ulrich	Co-I	University of California, Los Angeles	Magnetic Field Calibration Code	Solar Cycle
Alan Wray	Co-I	NASA Ames Research Center	Convection Zone MHD Model Code	Convection Physics
^* Deceased

HMI Science Team - International Co-Is
Name	Role	Institution	Phase B,C,D	Phase-E
HMI International Co-Investigators
J. Christensen-Dalsgaard	Co-I	TAC, Aarhus University, DK	Solar Model Code	Helioseismology
J. Leonard Culhane	Co-I	MSSL, University College London, UK		Active Region Science
Bernhard Fleck	Co-I	European Space Agency	ILWS Coordination	Atmospheric Dynamics
Douglas O. Gough	Co-I	IoA, Cambridge University, UK	Local HS Inversion Code	Helioseismology
Richard A. Harrison	Co-I	Rutherford Appleton Laboratories, UK		Active Region Science
Takashi Sekii	Co-I	National Astron. Obs. of Japan, JP		Helioseismology
Hiromoto Shibahashi	Co-I	University of Tokyo, JP		Helioseismology
Sami K. Solanki	Co-I	Max-Planck-Institut für Aeronomie, DE		AR Science
Michael J. Thompson	Co-I	Imperial College, UK		Helioseismology

Updated 15 Nov 2011.

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