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Plasma Parameters and Structures of the X4 Flare of 19 May 1984 as Observed by SMM-XRP

Published online by Cambridge University Press:  27 September 2017

J.T. Schmelz ,
J.L.R. Saba  and
K.T. Strong
J.T. Schmelz
Affiliation:
Applied Research Corporation under subcontract to Lockheed PARL
J.L.R. Saba
Affiliation:
Lockheed Palo Alto Research Laboratory
K.T. Strong
Affiliation:
Lockheed Palo Alto Research Laboratory

Abstract

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The eruption of a large flare on the east limb of the Sun was observed by the X-Ray Polychromator (XRP) on board the Solar Maximum Mission (SMM) on 19 May 1984. The XRP Flat Crystal Spectrometer (FCS) made polychromatic soft X-ray images during the preflare, flare and postflare phases. The XRP Bent Crystal Spectrometer (BCS) provided information on the temperature and dynamics of the hot (Te > 8 x 106K) coronal plasma from spectra integrated spatially over the whole region.

Type
Session II: Solar Flares
Information
International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 165 - 168
Copyright
Copyright © Kluwer 1989

References

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