VLA, PHOENIX, and BATSE observations of an X1 flare

Details VLA, PHOENIX, and BATSE observations of an X1 flare VLA, PHOENIX, and BATSE observations of an X1 flare

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992nascp3137..515w&link_type=abstract

In its The Compton Observatory Science Workshop p 515-521 (SEE N92-21874 12-90)

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Coronas, Gamma Ray Observatory, Radio Spectroscopy, Solar X-Rays, Type 3 Bursts, Type 4 Bursts, Very Large Array (Vla), Drift Rate, Scale Height, Solar Magnetic Field, Unsteady Flow

Scientific paper

We present observations of an X1 flare (18 Jul. 1991) detected simultaneously with the Very Large Array (VLA), the PHOENIX Digital Radio Spectrometer and the Burst and Transient Source Experiment (BATSE) aboard the Gamma Ray Observatory (GRO). The VLA was used to produce snapshot maps of the impulsive acceleration in the higher corona several minutes before the onset of the hard x ray burst detected by BATSE. Comparisons with high spectral and temporal observations by PHOENIX reveal a variety of radio bursts at 20 cm, such as type 3 bursts, intermediate drift bursts, and quasi-periodic pulsations during different stages of the X1 flare. From the drift rates of these radio bursts we derive information on local density scale heights, the speed of radio exciters, and the local magnetic field. Radio emission at 90 cm shows a type 4 burst moving outward with a constant velocity of 240 km/s. The described X1 flare is unique in the sense that it appeared at the east limb (N06/E88), providing the most accurate information on the vertical structure of different flare tracers visible in radio wavelengths.

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