Meter-decameter observations of dMe flare stars with the Clark Lake Radio telescope

Details Meter-decameter observations of dMe flare stars with the Clark Lake Radio telescope Meter-decameter observations of dMe flare stars with the Clark Lake Radio telescope

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..130..391j&link_type=abstract

(Committee of European Radio Astronomers, SNSF, URSI, et al., Workshop on Particle Beams in the Solar Atmosphere, Braunwald, Swi

Astronomy and Astrophysics

Astronomy

5

Dwarf Stars, Flare Stars, M Stars, Radio Astronomy, Stellar Flares, Antenna Arrays, Decametric Waves, Solar Radio Emission, Very Large Array (Vla)

Scientific paper

The now-closed Clark Radio Observatory was used in 1984 and 1985 to search for flaring emission from a number of dMe flare stars in the 30.9 to 110.6 MHz frequency range. No emission was found to greatly exceed detection limits which range from about 1 Jy for 1 hr averaging, to about 50 Jy for 1 s averaging, even though flares were often seen to tens of mJy at 20 cm using the VLA for those times when VLA-CLRO observations were coordinated. There are marginal detections of flaring from AD Leo over two periods on December 15, 1985 which mark the beginning and the end of a long-lasting, narrow-band flare at 1415 MHz.

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