Coronal Flares -- Cycle 1

Details Coronal Flares -- Cycle 1 Coronal Flares -- Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1158m&link_type=abstract

HST Proposal ID #1158

Computer Science

Hst Proposal Id #1158

Scientific paper

We will observe coronal flares in AU Mic with the HRS. Spectral coverage is traded in favor of time resolution; a single grating setting in medium resolution mode, however, allows us to observe emissions from Fe XXI, Fe XII, and O V, so that the emissions from flare plasmas at 1E7 K, 1.6E6 K, and 2.5E5 K can be compared. The same setting allows us to monitor bright lines of O I and C I, so that coronal flares can be related to activity in the 10,000 K plasma. Groundbased observations will be scheduled to determine the response of photospheric gas to the coronal flare; radio and X-ray observations will also be arranged or solicited if possible.

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