Trace — The transition region and coronal explorer

Details Trace — The transition region and coronal explorer Trace — The transition region and coronal explorer

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..119s&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 119-122

Physics

13

Sun, Instrumentation, Coronal Heating, Coronal Structure

Scientific paper

TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from 104 to 107 K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena.

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