Future Capabilities for Solar/Stellar Observations
Ken Carpenter, Don Hassler, Tom Berger, Tim Bastian, Roberto Pallavicini, & Suchitra Balachandran

Institute: Goddard Space Flight Center
Institute: Southwest Reasearch Institute
Institute: Lockheed Martin Solar and Astrophysics Lab
Institute: NRAO
Institute: INAF/Osservatorio Astronomico di Palermo
Institute: University of Maryland
Contact Email: kgc@stargate.gsfc.nasa.gov

PDF FILES

Future Capabilities for Solar/Stellar Observations (Full session - 224 pages) [PDF]

Hassler -- Space-Based Solar Physics (35 pages) [PDF]

Berger -- Ground-Based Solar Optical Observations (42 pages) [PDF]

Bastian -- Future Instrumentation for Solar and Stellar Research At Radio Wavelengths (43 pages) [PDF]

Carpenter -- Space-Based Stellar Observations (44 pages) [PDF]

Pallavicini -- Ground-Based Optical Instrumentation for Stellar Studies (43 pages) [PDF]

Balachandran -- Ground-Based Stellar Infrared Instrumentation (16 pages) [PDF]

POWERPOINT FILES

Future Capabilities for Solar/Stellar Observations (Introduction - 1 page) [PPT]

Hassler -- Space-Based Solar Physics (35 pages) [PPT]

Berger -- Ground-Based Solar Optical Observations (42 pages) [PPT]

Bastian -- Future Instrumentation for Solar and Stellar Research At Radio Wavelengths (43 pages) [PPT]

Carpenter -- Space-Based Stellar Observations (44 pages) [PPT]

Pallavicini -- Ground-Based Optical Instrumentation for Stellar Studies (43 pages) [PPT]


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Manuscript submitted: 2001-Sep-3
"The Future of Cool-Star Astrophysics", 2003, Eds. A. Brown, G. M. Harper, & T. R. Ayres. Proceedings of 12th Cambridge Workshop on Cool Stars, Stellar Systems, & The Sun,
© 2003 University of Colorado.