Observations of Different Type of Bursts Associated with M 6.3 Solar Flares

Abstract

Variation of solar bursts due to solar flares such as type an isolated type III , a complex type III, U is being highlighted. These bursts occurred on 9th March 2012 at the National Space Centre, Sg. Lang, Selangor, Malaysia Here, we study a unique case with a combination of two types burst associated with solar flare and CMEs. Our observation is focused on the low frequency region starting from 150 MHz till 400 MHz. We found that a solar flare type solar flare type M 6.3 which occurred in active region AR 1429 starting from 3:32 UT and ending at 05:00 UT. The flare has been confirmed to be the largest flare since 2005. Some physical parameters will be measured. We then compared our results with X-ray data from NOAA Space Weather Prediction Centre (SWPC).

Solar Radio Burst Data Processing of CALLISTO and Frequency Drift Rate Determination of Solar Radio Burst Detected by CALLISTO Network in Indonesia

“…On the other hand, in this stage can be considered as pre-flare which could be a signature of accelerated electrons [18] as evidenced by found that 60% of the drift (type III) bursts of solar radio synchronized at the same time with the solar flare [19]. In addition, the dynamic structure of Type III solar radio bursts known as ejection of local plasma oscillations due to interference of atoms excitation in radiation of incoherent plasma frequency such as gyro synchrotron and emission-free that appear in radio wavelengths dominant in the meter and decimeter [20,21]. Type III bursts commonly occur early in the rise of impulsive solar flares may indicate that open field lines are important parts of model for release energy by magnetic fields such as flares [22,23].…”

Preliminary Analysis on the Solar Burst Type III and the Effect of the Magnetic Reconnection

“…These forces drive the plasma to a state unstable to the growth the beam-plasma interactions, is believed to generating these waves [22,23]. This type is very synonymous at the meter and decimeter wavelengths [24,25]. Early stage of solar flares may indicate that open field lines are an essential part of models for energy release by magnetic fields [26,27].…”

Preliminary Analysis on the Solar Burst Type III and the Effect of the Magnetic Reconnection

“…These forces drive the plasma to a state unstable to the growth the beam-plasma interactions, is believed to generating these waves [22,23]. This type is very synonymous at the meter and decimeter wavelengths [24,25]. Early stage of solar flares may indicate that open field lines are an essential part of models for energy release by magnetic fields [26,27].…”