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Review of RF15-I X-ray photometer observations View all abstracts by submitter

Marek Siarkowski   Submitted: 1999-11-26 15:01

RF15-I is a joint Czech-Polish Solar Soft/Hard X-ray broad-band photometer aboard the INTERBALL-Tail Probe satellite. By observing the Sun (since August 1995) in the energy bands: 2-3-5-8 and 10-15-30-60-120-240 keV, this photometer provides complementary data to GOES, BATSE and YOHKOH/HXT. Here, we present examples of reduced high-time resolution observations for several flares observed. These observations will be used subsequently in order to study flare energetics, statistics and diagnostics of the flare acceleration processes. Determination of important plasma parameters is envisaged. The data may support also the analysis of magnetospheric plasma.

Authors: Siarkowski, M., Sylwester, J., Gburek, S. and Kordylewski, Z.

Publication Status: in Proc. of the Ninth European Meeting on Solar Physics, ``Magnetic Fields and Solar Processes'', Florence, Italy, 12-18 Septemb
Last Modified: 1999-11-26 15:01
Go to main E-Print page  LASCO Measurements of the Energetics of Coronal Mass Ejections
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