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