Nv. Baranov et Li. Tsvetkov, PULSATIONS IN MICROWAVE-BURSTS FROM 2 SOURCES DURING SOLAR-FLARES ON JULY 11, 1991, Astronomy letters, 20(3), 1994, pp. 327-331
The results of observations of two solar-active regions at wavelengths
of 3.5, 2.8, 2.25, and 1.95 cm with the 22-meter radio telescope of t
he Crimean Astrophysical Observatory are presented. The comparative an
alysis of polarized radio emission of the active regions allowed us to
identify a sympathetic burst with pulsations from the source, located
at a distance of L greater-than-or-equal-to 4 x 10(5) km from the sit
e of initial flare. Dynamic Fourier-spectra of the radio emission puls
ations of the interacting active regions contained reliable components
at frequencies 0.029, 0.033, and 0.045 Hz, as well as their second ha
rmonics. A density-modulated stream of energetic (epsilon > 10 keV) el
ectrons, moving with velocities approximately 6 x 10(4) km s-1 inside
the coronal magnetic arc that connected the two active regions, is ass
umed to be the trigger of the sympathetic burst.