V.F. Melnikov1,2
and A.V.R. Silva 2
1 Radiophysical Research
Institute, B.Pecherskaya St. 25, 603600, Nizhnii Novgorod, Russia
2 CRAAE, Mackenzie, R. da Consolação, 896, 01302-000, São, Paulo, Brazil
In this work the relation and temporal evolution
of spectral indices of relatively weak impulsive HXR- and microwave bursts
are investigated. The study has been done using the data obtained in 1991-1994
with BATSE and OVRO. The frequency range covered by OVRO is 1-18 GHz. Hard
X-ray emission above the background for most of the events ranges from
20 to 200 keV. An interesting new result is that most of the events presents
continuous microwave spectral flattening (in the optically thin region
(at f>fp)) simultaneously with softening of HXR-spectrum during
the decay phase. In the case of hardening or no changes in the HXR-spectrum
the microwave spectrum flattens. On the other hand, almost all events which
display a steepening of the microwave spectrum also display a softening
of the HXR-spectrum. It is shown that in the majority of the events during
the rise phase and at the time of maximum of the bursts the difference
=
x
µ
between electron spectral indices derived from HXR-spectra and microwave
spectra is in the range 0.5-1.5. However, in some cases
can reach 2-3. In most of the events
increases in the decay phase, reaching in some events the value of 4-6.
We show that the differences between
x
and
µ
and their temporal change during the decay phase can be naturally explained
mainly by the dynamics of the energy spectrum of trapped electrons due
to Coulomb collisions and wave-particle interactions. We simulated the
microwave and HXR spectrum evolution assuming that the electron injection
spectrum hardens during the rise phase and softens during the decay phase
(`soft-hard-soft' behavior). Simulations show that when the spectrum of
accelerated electrons during the decay phase softens at all energies, the
spectrum of trapped electrons softens only at low energies. At high energies
the trapped electron spectrum hardens with time causing the continuous
spectral flattening of microwave emission at high frequencies (in optically
thin region). The value of the `break-up' energy depends on the injection
duration and conditions in a flare loop.