activity
20172022
most citedCharacteristics of events with metric-to-decahectometric type II radio bursts associated with CMEs and flares in relation to SEP events

12 citations · 19 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20223 cited

Kinematic study of radio-loud CMEs associated with solar flares and DH type II radio emissions during solar cycles 23 and 24

P. Pappa Kalaivani, O. Prakash, A. Shanmugaraju +2

We have statistically analyzed 379 radio-loud (RL) CMEs and their associated flares during the period 1996 - 2019 covering both solar cycles (SC) 23 and 24. We classified them into…

astro-ph.SR2021

Analysis of type II and type III radio bursts associated with SEPs from non-interacting/interacting radio-loud CMEs

P Pappa Kalaivani, O Prakash, A Shanmugaraju +4

We analyze radio bursts observed in events with interacting/non-interacting CMEs that produced major SEPs (Ip 10 MeV) fromApril 1997 to December 2014.We compare properties of m…

astro-ph.SR2021

Occurrence rate of radio-loud and halo CMEs in solar cycle 25: Prediction using their correlation with sunspot numbers

A. Shanmugaraju, P. Pappa Kalaivani, Y. -J. Moon +1

The coronal mass ejections (CMEs) from the Sun are known for their space weather and geomagnetic consequences. Among all CMEs, so-called radio-loud (RL) and halo CMEs are considere…

astro-ph.SR20204 cited

Statistical characteristics on SEPs, radio-loud CMEs, low frequency type II and type III radio bursts associated with impulsive and gradual flares

P. Pappa Kalaivani, A. Shanmugaraju, O. Prakash +1

We have statistically analyzed a set of 115 low frequency (Deca- Hectometer wavelengths range) type II and type III bursts associated with major Solar Energetic Particle (SEP: Ep >…

astro-ph.SR201712 cited

Characteristics of events with metric-to-decahectometric type II radio bursts associated with CMEs and flares in relation to SEP events

O. Prakash, Li Feng, G. Michalek +4

A gradual solar energetic particle (SEP) event is thought to happen when particles are accelerated at a shock due to a fast coronal mass ejection (CME). To quantify what kind of so…