activity
20172022
most citedEarly-Stage SEP Acceleration by CME-Driven Shocks with Realistic Seed Spectra: I. Low corona

14 citations · 14 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022

Multi-Scale Image Preprocessing and Feature Tracking for Remote CME Characterization

Oleg Stepanyuk, Kamen Kozarev, Mohamed Nedal

Coronal Mass Ejections (CMEs) influence the interplanetary environment over vast distances in the solar system by injecting huge clouds of fast solar plasma and energetic particles…

astro-ph.SR2022

A Multi-Event Study of Early-Stage SEP Acceleration by CME-Driven Shocks -- Sun to 1 AU

Kamen Kozarev, Mohamed Nedal, Rositsa Miteva +2

The solar corona below 10 solar radii is an important region for early acceleration and transport of solar energetic particles (SEPs) by coronal mass ejection-driven shock waves. T…

astro-ph.SR2019

Comprehensive Characterization of Solar Eruptions With Remote and In-Situ Observations, and Modeling: The Major Solar Events on 4 November 2015

Iver H. Cairns, Kamen A. Kozarev, Nariaki V. Nitta +12

Solar energetic particles (SEPs) are an important product of solar activity. They are connected to solar active regions and flares, coronal mass ejections (CMEs), EUV waves, shocks…

astro-ph.SR201914 cited

Early-Stage SEP Acceleration by CME-Driven Shocks with Realistic Seed Spectra: I. Low corona

Kamen Kozarev, Maher A. Dayeh, Ashraf Farahat

An outstanding problem in heliospheric physics is understanding the acceleration of solar energetic particles (SEP) in coronal mass ejections (CMEs) and flares. A fundamental quest…

astro-ph.IM2018

Solar Imaging using Low Frequency Arrays

C. Lonsdale, L. Benkevitch, I. Cairns +8

Low frequency imaging radio arrays such as MWA, LWA and LOFAR have been recently commissioned, and significantly more advanced and flexible arrays are planned for the near term. Th…

astro-ph.SR2017

The Coronal Analysis of SHocks and Waves (CASHeW) Framework

K. Kozarev, A. Davey, A. Kendrick +2

Coronal Bright Fronts (CBF) are large-scale wavelike disturbances in the solar corona, related to solar eruptions. They are observed in extreme ultraviolet (EUV) light as transient…