4 papers
A type II solar radio burst without a coronal mass ejection association
Anshu Kumari, Nat Gopalswamy
Type II solar radio bursts are commonly associated with shocks generated by coronal mass ejections (CMEs), where plasma waves are excited by magnetohydrodynamic (MHD) processes and…
Insights into Chromospheric Large-Scale Flows using Nobeyama 17 GHz Radio Observations I. The Differential Rotation Profile
Srinjana Routh, Anshu Kumari, Vaibhav Pant +4
Although the differential rotation rate on the solar surface has long been studied using optical and extreme ultraviolet (EUV) observations, associating these measurements to speci…
CME-associated type-IV radio bursts: The solar paradigm and the unique case of AD Leo
Atul Mohan, Nat Gopalswamy, Surajit Mondal +2
The type-IV bursts, associated with coronal mass ejections (CMEs), occasionally extend to the decameter-hectrometric (DH) range. We present a comprehensive catalog of simultaneous…
Inter-planetary type-IV solar radio bursts: A comprehensive catalog and statistical results
Atul Mohan, Nat Gopalswamy, Anshu Kumari +2
Decameter hectometric (DH; 1-14 MHz) type-IV radio bursts are produced by flare-accelerated electrons trapped in post-flare loops or the moving magnetic structures associated with…