Issue |
A&A
Volume 437, Number 3, July III 2005
|
|
---|---|---|
Page(s) | 1047 - 1054 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20042578 | |
Published online | 30 June 2005 |
Recent data on zebra patterns
1
National Astronomical Observatory, Chinese Academy of Science, 20A, Datun Road, Beijing, 100012, PR China e-mail: yyh@bao.ac.cn
2
Izmiran, Troitsk, Moscow region, 142190, Russia e-mail: gchernov@izmiran.rssi.ru
Received:
20
December
2004
Accepted:
13
February
2005
A comparative analysis of two recent solar radio outbursts around
3 GHz with zebra structures and fiber bursts in their dynamical
radio spectra is carried out using all available ground-based and
satellite data (SOHO, TRACE, RHESSI). The latest theoretical models
of the zebra pattern are critically discussed.
New data on microwave zebra structures and fiber bursts suggests
that they are analogous to similar structures observed at meter
wavelengths. It was discovered that in the 2,6–3,8 GHz frequency
band more than 34 zebra stripes can appear simultaneously, and
some isolated fiber bursts can continuously be transformed into
zebra stripes. This fact indicates a single origin for both
structures. The zebra pattern was observed when the signs of
magnetic reconnections were revealed in images of 195 Å UV lines, and radio sources coincided with positions of some new sources in hard X-rays. All the main properties of the
stripes in emission and absorption can be explained if they are
associated with interactions between electrostatic plasma waves
and whistlers, taking into account the quasi-linear diffusion of
fast particles with the loss-cone distribution on whistlers. In
this model it is possible to obtain realistic values for the
magnetic field strength of at the plasma level
of about 3 GHz. The double plasma resonance model for the zebra
pattern based on the known realistic dependences of electron
density and magnetic field yields a frequency dependence for the
frequency separation between stripes that does not agree with the
observations.
Key words: Sun: flares / Sun: radio radiation / Sun: activity / Sun: UV radiation
© ESO, 2005
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