On the Zebra Structure in the Frequency Range near 3 GHz
- 1 December 2001
- journal article
- Published by IOP Publishing in Chinese Journal of Astronomy and Astrophysics
- Vol. 1 (6) , 525-536
Abstract
We present 19 cases of zebra pattern structure (ZPS) and fiber bursts (FB) in radio bursts in frequency range around 3GHz, and one such case in the range 5.2-7.6GHz, using the new microwave spectrometer of NAOC between 2.6- 3.8 and 5.2-7.6GHz (China, Huairou station) with high resolution (10MHz and 8ms). The FB and ZPS have about the same spectral parameters: the frequency bandwidth of emission stripes f 20MHz, the frequency separation between the emission and the neighboring low frequency absorption fea 30MHz and the frequency separation between emission stripes (when a periodic structure persists) fs 60-70MHz. Therefore we consider both these fine structures to be whistler manifestations, i.e., interactions of plasma electrostatic waves with whistler waves (generated by the same fast particles with loss-cone anisotropy) l + w ! t. The duration of the fiber bursts of about 2s corresponds to whistler waves propagat- ing undamped at about 2s, which requires a whistler increment < 0.5 s 1. In the frequency range 3-7GHz the relation between the ratios of plasma to cyclotron frequencies and whistler to cyclotron frequencies is almost independent of the decre- ment of whistler electron damping. This finding is used to obtain the magnetic field strength in the region of generation. For a reasonable value of electron temperature (2-20MK), we find B = 125 190G when the electron density is (8 18)◊1010 cm 3 and B = 520 610G when the electron density is (35-60)◊1010 cm 3. In two re- markable events, 1998-04-15 and 2000-10-29, the right-hand polarization is strong for all the fine structures and corresponds to ordinary wave.Keywords
This publication has 12 references indexed in Scilit:
- Solar Radio Radiation Bursts on 1998 April 15Publications of the Astronomical Society of Japan, 2000
- Delay between the circularly polarized components in fine structures during solar type IV eventsSolar Physics, 1995
- Magnetospheres of Solar Active Regions Inferred from Spectral-Polarization Observations with High Spatial ResolutionThe Astrophysical Journal, 1993
- Soft X-ray spectroscopy of solar flares - an overviewThe Astrophysical Journal Supplement Series, 1990
- On the intermediate drift burst modelSolar Physics, 1987
- The electron-cyclotron maser instability as a source of plasma radiationThe Astrophysical Journal, 1986
- Interpretation of patterns of drifting Zebra stripesSolar Physics, 1983
- Generation of intermediate drift bursts in solar type IV radio continua through coupling of whistlers and Langmuir wavesSolar Physics, 1975
- Cyclotron wave instability in the corona and origin of solar radio emission with fine structureSolar Physics, 1975
- Cyclotron Wave Instabilities in a PlasmaThe Physics of Fluids, 1967