Astronomy and Astrophysics – Astronomy
Scientific paper
May 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsh33a..13v&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SH33A-13
Astronomy and Astrophysics
Astronomy
6954 Radio Astronomy, 7534 Radio Emissions, 7536 Solar Activity Cycle (2162)
Scientific paper
Type II and III solar radio bursts have been observed for more than 50 years. Several theories suggest that the basic emission mechanisms of these two types of bursts are similar with the exception of a few sub-classes of type II bursts. Research in the 2 GHz range has shown that the average frequency of occurrence of type II solar bursts closely follows the solar cycle over a time span of roughly 40 years. Ground based observations of type II and III solar radio burst emissions suggest similar behavior. Data taken at 20.1 MHz between February 2005 and February 2006 using a narrow band receiver has been averaged weekly and monthly and then been compared to the 2 GHz data timeline. Upon comparison it is evident that the two data sets show similar periodicities. We demonstrate the relationship between the 20.1 MHz solar cyclotron emissions and the 2 GHz synchrotron emissions and show that the 20.1 MHz data follows the solar cycle.
Higgins C.
Mason Paolo
Villarreal M.
No associations
LandOfFree
Solar Cycle Variability of Low Frequency Solar Radio Emission does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Solar Cycle Variability of Low Frequency Solar Radio Emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Cycle Variability of Low Frequency Solar Radio Emission will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1026645