Analysis of solar type II radio bursts in conjunction with multi-wavelength
observations
A. Shanmugaraju
Abstract
The Sun was continuously monitored in the frequency range 30-80 MHz on
a regular basis using the new radio spectrograph (Madurai Solar Radio Spectrograph,
MSRS) which is now located at the Radio Astronomy Centre, Ooty. We have
collected data on various types of solar radio bursts using this spectrograph.
In the present work, ten type II bursts observed during March - April 1998
and August 1998 have been analysed in conjunction with other ground based
observations from Culgoora and Hiraiso. The associated activities have
also been investigated using multi-wavelength observations obtained from
YOKOH, LASCO and WAVE. Comparison with LASCO data reveal that, while most
of the bursts in our sample are associated with energetic flares
on the Sun, there are a few that may have been associated with CMEs/bright
front features. Comparison with WAVE data reveal that, while in general,
the dynamic spectrum do not extend below 25 MHz or so, there are instances
where the type II dynamic spectrum can be seen extending down to the WAVE
spectrum.
Authors: A. Shanmugaraju and S.
Umapathy
Organization: Madurai Kamaraj University
Telephone: ?
Fax: ?
e-mail: shanmug@racooty.ernet.in
Address: Radio Astronomy Centre
Post Box No.8
Ooty - 643 001.