Relationship between solar radio spikes observed at 1420 MHz and solar active phenomena

Details Relationship between solar radio spikes observed at 1420 MHz and solar active phenomena Relationship between solar radio spikes observed at 1420 MHz and solar active phenomena

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..491d&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Physics

1

Solar Activity: Solar Radio Spikes

Scientific paper

Numerous solar radio narrow-band spikes have been observed with the RT-15 radio telescope of Toruń Observatory between March 15, 2000 and May 14, 2001. We present here a brief description of three interesting events (from 11 events collected during 2000 hours of observations) and first results of analysis of the relationship between the spikes, solar flares and coronal mass ejections. We have found that solar spikes were emitted from solar flares of various scenario of evolution and various configuration of the interacting magnetic fields. Moreover, some groups of spikes were not correlated in time with any solar flare recorded by GOES or Yohkoh. It is very interesting to note, that on the basis of the GOES database merely 2% of the solar flares emit the radio spikes.

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