HR: 0800h
AN: SH21B-0413    [Abstracts]
TI: STEREO in the Virtual Solar Observatory Context
AU: * Hourcle, J A
EM: joseph.a.hourcle.1@gsfc.nasa.gov
AF: L3/NASA-GSFC, Code 682.3 NASA-GSFC, Greenbelt, MD 20771 United States
AU: Bogart, R
EM: rbogart@spd.aas.org
AF: Stanford U., Center for Space Science and Astrophysics Stanford University, Stanford, CA 94305 United States
AU: Davey, A
EM: ard@boulder.swri.edu
AF: SwRI, 1050 Walnut Street, Suite 400, Boulder, CO 80302 United States
AU: Gurman, J B
EM: gurman@gsfc.nasa.gov
AF: NASA-GSFC, Code 682.3 NASA-GSFC, Greenbelt, MD 20771 United States
AU: Hill, F
EM: hill@noao.edu
AF: NOAO, 950 North Cherry Avenue, Tucson, AZ 85719 United States
AU: Martens, P
EM: martens@mithra.physics.montana.edu
AF: NOAO, 950 North Cherry Avenue, Tucson, AZ 85719 United States
AU: Suarez-Sola, I
EM: igor@noao.edu
AF: MSU-Bozeman, Department of Physics Montana State University, Bozeman, MT 59717 United States
AU: Tian, K
EM: ktian@stanford.edu
AF: Stanford U., Center for Space Science and Astrophysics Stanford University, Stanford, CA 94305 United States
AU: Yoshimura, K
EM: yosimura@mithra.physics.montana.edu
AF: MSU-Bozeman, Department of Physics Montana State University, Bozeman, MT 59717 United States
AB: The Virtual Solar Observatory (VSO) was designed with the goal that it handle heterogeneous data sets from multiple observatories. With its two spacecraft and multiple instruments, the STEREO mission provides an excellent example of solar physics research based on multiple data sets, and a good test of the abilities of the VSO. Here we will discuss how the VSO will meet the key challenges that STEREO presents. In particular, the wide range of data classes and the non-stationary viewpoints of the two spacecraft demand a flexible underlying data model of the VSO.
UR: http://www.virtualsolar.org/
DE: 7599 General or miscellaneous
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2004 AGU Fall Meeting