The Variance Formation of M9.3 Solar Flare Associated with Solar Radio Burst Type V Occurred at Eight (8) Different Sites of the CALLISTO System on 4th August 2011

Abstract

We report a detailed examination of the variance formation of M9.3 solar flare associated with solar radio burst Type V that occurred on 2011 August 4. Solar radio burst type V was identified occurred with present of Coronal Mass Ejection (CME) towards earth which moving estimated about 1,950 km/s which can gives major impact to our Earths in terms of satellites. The event was observed by using Compound Astronomical Low-cost Low-Frequency Instrument for Spectroscopy Transportable Observatory (CALLISTO). CALLISTO is a radio spectrometer that has been used 24 hour per day which designed for solar observation. The solar radio burst was occurred at 21.1 MHz at 3 minutes (0358 UTC till 0401 UTC). Noted that all the sites are less suffering from local RFI with solar wind speed and density reached 411.6 km/sec and 3.8 proton/cm3. Solar radio burst Type V is known as smooth with short-lived continuum which sometime followed by a type III burst. We show radio flux density in eight (8) different sites. Finally, we discuss the X-ray flux density to determine classes of the solar flares.