The Beginning Impulsive of Solar Burst Type IV Radio Emission Detection Associated with M Type Solar Flare

Authors: Z.S. Hamidi, Z.Z. Abidin, Z.A. Ibrahim, C. Monstein, N.N.M. Shariff, M. Sabaghi

Affiliations: Faculty of Science, University Malaya, 50603 Kuala Lumpur, Malaysia, Institute for Astronomy, ETH Zurich, Switzerland

Emails: [email protected]

Journal: International Journal of Fundamental Physical Sciences (IJFPS)

Volume: 2, Issue: 2, Pages: 29-31, Date: June, 2012

ISSN: 2231-8186

DOI: https://doi.org/10.14331/ijfps.2012.330031

Abstract

First light detection of solar burst type IV in Malaysia in the region of 260 MHz to 380 MHz was successfully observed on 5th March 2012, associated with an M2.0 class solar flare. The burst's variation suggests effects of magnetic reconnection potentially inducing disturbances in Earth's magnetotail. This research, part of the International Space Weather Initiative (ISWI), marks the beginning of Malaysia's participation in solar radio emission monitoring using CALLISTO spectrometer and LPDA at the National Space Centre.

Keywords

Solar burst type IV, Solar flare, Sunspot, CALLISTO

License: https://creativecommons.org/licenses/by/4.0/