7 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…
Role of CME clusters and CME-CME interactions in producing sustained -ray emission
Atul Mohan, Pertti Makela, Natchimuthuk Gopalswamy +2
Fast (V>1000) coronal mass ejections (CMEs) capable of accelerating protons beyond 300MeV are thought to trigger hours-long sustained -ray emiss…
Results from NASA's First Radio Telescope on the Moon: Terrestrial Technosignatures and the Low-Frequency Galactic Background Observed by ROLSES-1 Onboard the Odysseus Lander
Joshua J. Hibbard, Jack O. Burns, Robert MacDowall +8
Radiowave Observations on the Lunar Surface of the photo-Electron Sheath instrument (ROLSES- 1) onboard the Intuitive Machines' Odysseus lunar lander represents NASA's first radio…
Novel scaling laws to derive spatially resolved flare and CME parameters from sun-as-a-star observables
Atul Mohan, Natchimuthuk Gopalswamy, Hemapriya Raju +1
Coronal mass ejections (CMEs) are often associated with X-ray (SXR) flares powered by magnetic reconnection in the low-corona, while the CME shocks in the upper corona and interpla…
A catalog of multi-vantage point observations of type-II bursts: Statistics and correlations
Atul Mohan, Nat Gopalswamy, Hemapriya Raju +1
Coronal mass ejection (CME) often produces a soft X-ray (SXR) flare associated with the low-coronal reconnection and a type-II radio burst associated with an interplanetary (IP) CM…
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…