High spatial resolution observations of solar flares at 3.3 mm wavelength

M. R. Kundu, S. M. White, W. J. Welch, John H Bieging

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

We present the first high-spatial-resolution interferometric observations of solar flares at millimeter wavelengths, carried out with the Berkeley-Illinois-Maryland Array (BIMA). The observations represent an improvement of an order of magnitude in both sensitivity and spatial resolution compared with previous solar observations at these wavelengths. Most of the flares occurring within the field of view during the observations were detected by BIMA, including both very impulsive and longer-duration events. It appears that millimeter burst sources are not much smaller than microwave sources. If the emission in the flash phase is predominantly due to gyrosynchrotron emission, we can rule out thermal gyrosynchrotron models for the radio emission because the flux at millimeter wavelengths is too high. During the Flares 22 campaign we will collect both imaging data as well as dedicated patrol observations of flare time profiles at millimeter wavelengths.

Original languageEnglish (US)
Pages (from-to)91-94
Number of pages4
JournalAdvances in Space Research
Volume11
Issue number5
StatePublished - 1991
Externally publishedYes

Fingerprint

solar flares
spatial resolution
wavelength
Wavelength
high resolution
flares
wavelengths
patrols
field of view
radio emission
Microwaves
flash
radio
Fluxes
bursts
Imaging techniques
microwaves
sensitivity
profiles

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

High spatial resolution observations of solar flares at 3.3 mm wavelength. / Kundu, M. R.; White, S. M.; Welch, W. J.; Bieging, John H.

In: Advances in Space Research, Vol. 11, No. 5, 1991, p. 91-94.

Research output: Contribution to journalArticle

Kundu, M. R. ; White, S. M. ; Welch, W. J. ; Bieging, John H. / High spatial resolution observations of solar flares at 3.3 mm wavelength. In: Advances in Space Research. 1991 ; Vol. 11, No. 5. pp. 91-94.
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