activity
20182026
most citedTesting two-component models on very-high-energy gamma-ray emitting BL Lac objects

33 citations · 56 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2026

Catalogue and statistics of greater than 100 MeV solar proton events during solar cycles 23-25 from SOHO-ERNE observations

M. Jarry, C. Palmroos, E. Lavasa +12

The SPEARHEAD (specification, analysis, and re-calibration of high-energy particle data) project, funded by the European Union Horizon Europe programme, enhances the accuracy and u…

astro-ph.SR2025

The high-energy protons of the ground level enhancement (GLE74) event on 11 May 2024

A. Papaioannou, A. Mishev, I. Usoskin +19

High energy solar protons were observed by particle detectors aboard spacecraft in near-Earth orbit on May 11, 2024 and produced the 74th ground level enhancement (GLE74) event reg…

astro-ph.SR2023

Separating the effects of earthside and far side solar events. A case study

Silja Pohjolainen, Nasrin Talebpour Sheshvan, Christian Monstein

On 8 November 2013 a halo-type coronal mass ejection (CME) was observed, together with flares and type II radio bursts, but the association between the flares, radio bursts, and th…

astro-ph.SR2023★ 10 cited

Self-consistent modeling of the energetic storm particle event of November 10, 2012

A. Afanasiev, R. Vainio, D. Trotta +4

It is thought that solar energetic ions associated with coronal/interplanetary shock waves are accelerated to high energies by the diffusive shock acceleration mechanism. For this…

astro-ph.SR2023★ 7 cited

On the Role of Interplanetary Shocks in Accelerating MeV Electrons

N. Talebpour Sheshvan, N. Dresing, R. Vainio +2

One of the sources of solar energetic particle (SEP) events is shocks that are driven by fast coronal mass ejections (CMEs). They can accelerate SEPs up to relativistic energies an…

astro-ph.SR2019★ 6 cited

Cut-off features in interplanetary solar radio type IV emission

Silja Pohjolainen, Nasrin Talebpour Sheshvan

Solar radio type IV bursts can sometimes show directivity, so that no burst is observed when the source region in located far from the solar disk center. This has recently been ver…