Published 1983 | Version v1
Journal article

SMM flat crystal spectrometer data analysis of 7 April 1980 flare

  • 1. Polska Akademia Nauk, Wroclaw. Centrum Badan Kosmicznych
  • 2. Wroclav Univ. (Poland). Astronomical Observatory
  • 3. Utrecht Univ. (Netherlands). Astronomical Inst., Space Research Lab.
  • 4. University Coll., London (UK). Mullard Space Science Lab.

Description

Soft X-ray images of the 1B/M4 flare of 7 April 1980 (start at 00:50 UT) recorded by Flat Crystal Spectrometer aboard Solar Maximum Mission satellite were analyzed. The X-ray flare consisted of two patches about 1 arcmin apart. Comparisons with magnetograms and white light images indicate that the two soft X-ray patches originate from two different loops or systems of loops. Systematic displacements of the brightest points of the patches are clearly seen during the flare development. For two selected resolution elements of the X-ray pictures (one element in each patch), a detailed differential emission measure analysis has been carried out and time evolution of the mean electron density and thermal energy content has been investigated. (author)

Additional details

Publishing Information

Journal Title
Publ. Debr. Heliophys. Obs. Hung. Acad. Sci.
Journal Volume
5
Journal Issue
1-3
Series
Publ. Debr. Heliophys. Obs. Hung. Acad. Sci.
Journal Page Range
85-92
ISSN
0209-7567

Conference

Title
11. conference on regional consultation on solar physics.
Dates
12-16 Sep 1983.
Place
Debrecen (Hungary).

INIS

Country of Publication
Hungary
Country of Input or Organization
Hungary
INIS RN
15065600
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ELECTRON DENSITY; IMAGE PROCESSING; ORBITING SOLAR OBSERVATORIES; SOLAR FLARES; SOLAR X-RAY BURSTS; SPATIAL DISTRIBUTION; X-RAY SPECTROMETERS
Descriptors DEC
DISTRIBUTION; MEASURING INSTRUMENTS; SATELLITES; SOLAR ACTIVITY; SPECTROMETERS; STELLAR FLARES

Optional Information

Notes
8 refs.; 3 figs.