Solar Physics Division Meeting 2000, June 19-22
Session 2. Corona, Solar Wind, Flares, CMEs, Solar-stellar, Instrumentation, Other
Display, Chair: J. Krall, Monday-Thursday, June 19, 2000, 8:00am-6:00pm, Forum Ballroom

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[2.44] First Results from the Upgraded Owens Valley Solar Array

D. E. Gary (New Jersey Institute of Technology), G. J. Hurford (UC Berkeley), Jeongwoo Lee, P. T. Gallagher (New Jersey Institute of Technology)

The Owens Valley Solar Array (OVSA) has undergone extensive hardware and software upgrades in preparation for the current solar maximum and the launch of HESSI. We present an overview of the now completed upgrade from 5 to 6 antennas, and show first results from the newly expanded instrument.

We show results from several recent flares, as well as multi-frequency maps of active region coronal structure, to demonstrate the improvements now possible with the instrument. The data and analysis software are freely available on the web, and we invite all who are interested in working with these data to contact the associated website.

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