Published 1984 | Version v1
Journal article

Simultaneous dual wavelength observations of an impulsive microwave burst using the V.L.A

  • 1. Indian Institute of Astrophysics, Bangalore

Description

Simultaneous observations of a microwave burst at 2 and 6 cm wavelengths were carried out with the Very Large Array (VLA). The 6 cm burst source is located close to a magnetic neutral line, presumably near the top of a flaring loop, while the 2 cm emission originates from the footpoints of the loop. It is concluded that the 6 cm emission is dominated by gyrosynchrotron radiation of the thermal electrons in the bulk heated plasma at a temperature of approximately 4 x 10 to the 7th K, while the 2 cm emission is due to nonthermal particles released and accelerated during the flare process. From the observed low degree of polarization and the lack of the 2 cm source cospatially with the 6 cm source a magnetic field of 200-350 G and delta approximately equal to or greater than 4 are estimated in the flare energy release site. A DC electric field flare model is invoked to explain the long delay between the peaks at the two wavelengths. From the delay, the strength of the electric field is estimated to be 0.2-4 micro statvolt/cm in the flaring region. 12 references

Additional details

Publishing Information

Journal Title
Adv. Space Res.
Journal Volume
4
Series
Adv. Space Res.
Journal Page Range
247-250
ISSN
0273-1177
CODEN
ASRSD

Conference

Title
25. plenary session of COSPAR.
Dates
25 Jun - 7 Jul 1984.
Place
Graz (Austria).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
17014579
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ELECTRIC FIELDS; PLASMA HEATING; SOLAR FLARES; SOLAR RADIO BURSTS; SYNCHROTRON RADIATION
Descriptors DEC
BREMSSTRAHLUNG; ELECTROMAGNETIC RADIATION; HEATING; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES

Optional Information

Secondary number(s)
CONF-8406167--.