Probability of Solar Flares Turn Out to Form a Coronal Mass Ejections Events Due to the Characterization of Solar Radio Burst Type II and III

ZS Hamidi - International Letters of Chemistry, Physics and …, 2014 - yadda.icm.edu.pl
The solar flare and Coronal Mass Ejections (CMEs) are well known as one of the most
massive eruptions which potentially create major disturbances in the interplanetary medium …

The Correlation between Solar Flare Phenomena in an X-ray Region and Radio Flux Measurement from January to September 2010

ZS Hamidi, NNM Shariff, MF Ali, C Monstein… - International Letters of …, 2014 - infona.pl
A short term variation of solar flare in nine months (January 2010 to September 2010) is
presented. This paper review and analyze the correlation between radio flux strength …

Analysis of slow partial Halo CME events with velocity of 100-200 km/s: an observation through CALLISTO system

NNM Shariff, ZS Hamidi… - … Conference on Industrial …, 2017 - ieeexplore.ieee.org
Halo event of coronal mass ejections (CMEs) had been once in a while reported in
coronagraph observations of the Sun before the Solar and Heliospheric Observatory …

Automatic solar radio burst type II and III image processing tracking by using CALLISTO system

ZS Hamidi, NNM Shariff - 2017 International Conference on …, 2017 - ieeexplore.ieee.org
Coronal Mass Ejections (CMEs) are well known as one of the most massive eruptions which
potentially create major disturbances in theinterplanetary medium and initiate severe …

The Mechanism of Signal Processing of Solar Radio Burst Data in E-CALLISTO Network (Malaysia)

ZS Hamidi, NNM Shariff - International Letters of Chemistry, Physics and …, 2014 - infona.pl
Solar space weather events like Coronal Mass Ejections and solar flares are usually
accompanied by solar radio bursts, which can be used for a low-cost real-time space …

The Non-thermal of a Large Solar Flares Associated with High Energy of Solar Burst Type III on 4th September 2017

ZS Hamidi, NNM Shariff - Journal of Physics: Conference Series, 2018 - iopscience.iop.org
On 4 th September 2017, the largest solar flare ever recorded this year saturated the GOES
satellite X-ray detectors, making an assessment of its size difficult. We report a large solar …

[PDF][PDF] Comparison of the Radio Frequency Interference (RFI) in the Region of Solar Burst Type III Data At Selected CALLISTO Network

ZS Hamidi, NNM Shariff… - International Letters of …, 2014 - bibliotekanauki.pl
Compact Astronomical Low-frequency, Low-cost Instrument for Spectroscopy in
Transportable Observatories (CALLISTO) is a global network of spectrometer system with …

[PDF][PDF] First Light Detection of A Single Solar Radio Burst Type III Due To Solar Flare Event

ZS Hamidi, NNM Shariff… - International Letters of …, 2014 - bibliotekanauki.pl
The eruption mechanism of solar flares and type III are currently an extremely active area of
research, especially during the solar cycle is towards maximum. In this case, the total energy …

Radio Observation of Coronal Mass Ejections (CMEs) Due to Flare Related Phenomenon on 7th March 2012

ZS Hamidi, C Monstein, NNM Shariff - International Letters of Chemistry …, 2014 - infona.pl
On March 7th, 2012, an active region AR1429 has unleashed 2 major X-class solar flares.
This flare is accompanied by a Coronal Mass Ejections (CMEs) event. A pair of unusually …

Automated solar radio burst detection on radio spectrum: a review of techniques in image processing

NZM Afandi, SN Hazmin, R Umar, AN Ishak - Journal of Fundamental and …, 2018 - ajol.info
The information of solar atmosphere was obtained after investigating the recording radiation
of the space mission. With technology growing recently, a lot of solar radio receiver was …