Multi-wavelength analysis of CME-driven shock and Type II solar radio burst band-splitting

It is now well established that Coronal Mass Ejections (CMEs) may produce shocks in near Sun and interplanetary medium. A Type-II radio burst is characterized by shock and associated emission with very slow frequency drift rate (∼0.1 MHz/sec). A CME driven shock and their velocity, acceleration/dece...

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Veröffentlicht in:	Astrophysics and space science 2021-03, Vol.366 (3), Article 31
Hauptverfasser:	Lata Soni, Shirsh, Ebenezer, E., lal Yadav, Manohar
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Astrobiology Astronomy Astrophysics Astrophysics and Astroparticles Coronal density Coronal mass ejection Cosmology Deceleration Drift rate Emissions Empirical analysis Frequency drift Interplanetary medium Magnetic fields Observations and Techniques Original Article Photovoltaic cells Physics Physics and Astronomy Radio emission Solar atmosphere Solar flares Solar radio bursts Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spectrographs Splitting Wavelengths
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