Highlights of the flare build-up study

Details Highlights of the flare build-up study Highlights of the flare build-up study

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..114..389g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 114, no. 2, 1987, p. 389-398.

Physics

11

Magnetohydrodynamic Stability, Solar Flares, Solar Radio Bursts, High Resolution, Magnetic Field Reconnection, Magnetohydrodynamic Shear Heating, Solar Cycles

Scientific paper

Years of preparation within the framework of the Flare Build-up Study (FBS) culminated in intensive observations of solar flares during the Solar Maximum Year (1979-1981). Scientists operating several spacecraft and roughly 70 ground-based observatories participated in an internationally coordinated effort to observe flares with higher spatial, spectral, and temporal resolution over a wider range of wavelengths than heretofore. The FBS stimulated important advances in theories of magnetic reconnection and the growth of plasma instabilities under preflare circumstances. A series of international FBS workshops facilitated data exchanges and collaborative studies for interpreting and synthesizing the wealth of new information about flares. The FBS ended officially at the Symposium on Synopsis of the Solar Maximum Analysis held July 2-5, 1986 at the COSPAR meeting in Toulouse, France. Here, highlights of its progress towards an understanding of the storage and release of preflare energy are summarized.

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