activity
20132026
most citedFirst year of energetic particle measurements in the inner heliosphere with Solar Orbiter's Energetic Particle Detector

69 citations · 276 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2026

Energetic Particle Acceleration and Transport: Interplanetary Coronal Mass Ejections and Shocks

Olga E. Malandraki, Christina M. S. Cohen, Joe Giacalone +16

Solar Energetic Particles from suprathermal (few keV) up to relativistic (few GeV) energies constitute an important contributor to the characterization of the space environment. Em…

astro-ph.SR2026

Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter

Xiaohang Chen, Gang Li, Joe Giacalone +12

The propagation of solar energetic particles (SEPs) through the heliosphere is primarily guided by the interplanetary magnetic field (IMF) which is embedded in the solar wind plasm…

astro-ph.SR2024

SEP environment in the inner heliosphere from Solar Orbiter and Parker Solar Probe

Robert F. Wimmer-Schweingruber, Javier Rodriguez-Pacheco, George C. Ho +4

The Sun drives a supersonic wind which inflates a giant plasma bubble in our very local interstellar neighborhood, the heliosphere. It is bathed in an extremely variable background…

astro-ph.SR2024★ 16 cited

The multi-spacecraft high-energy solar particle event of 28 October 2021

A. Kouloumvakos, A. Papaioannou, C. O. G. Waterfall +15

Aims. We studied the first multi-spacecraft high-energy solar energetic particle (SEP) event of solar cycle 25, which triggered a ground level enhancement (GLE) on 28 October 2021,…

astro-ph.SR2023

Solar Electron Beam -- Langmuir Wave Interactions and How They Modify Solar Electron Beam Spectra: Solar Orbiter Observations of a Match Made in the Heliosphere

Camille Y. Lorfing, Hamish A. S. Reid, Raul Gomez-Herrero +7

Solar Orbiter's four in-situ instruments have recorded numerous energetic electron events at heliocentric distances between 0.5 and 1au. We analyse energetic electron fluxes, spect…

astro-ph.SR2023

Modelling two Energetic Storm Particle Events Observed by Solar Orbiter Using the Combined EUHFORIA and iPATH Models

Zheyi Ding, Gang Li, Glenn Mason +6

By coupling the EUropean Heliospheric FORcasting Information Asset (EUHFORIA) and the improved Particle Acceleration and Transport in the Heliosphere (iPATH) model, two energetic s…

astro-ph.SR2023★ 50 cited

The 17 April 2021 widespread solar energetic particle event

N. Dresing, L. Rodríguez-García, I. C. Jebaraj +46

Context. A solar eruption on 17 April 2021 produced a widespread Solar Energetic Particle (SEP) event that was observed by five longitudinally well-separated observers in the inner…

astro-ph.SR2022★ 6 cited

Solar activity relations in energetic electron events measured by the MESSENGER mission

L. Rodríguez-García, L. A. Balmaceda, R. Gómez-Herrero +10

Aims. We perform a statistical study of the relations between the properties of solar energetic electron (SEE) events measured by the MESSENGER mission from 2010 to 2015 and the pa…

astro-ph.SR2022★ 20 cited

Solar energetic electron events measured by MESSENGER and Solar Orbiter. Peak intensity and energy spectrum radial dependences: statistical analysis

L. Rodríguez-García, R. Gómez-Herrero, N. Dresing +10

Context/Aims: We present a list of 61 solar energetic electron (SEE) events measured by the MESSENGER mission and the radial dependences of the electron peak intensity and the peak…

astro-ph.SR2022★ 6 cited

The first gradual solar energetic particle event with enhanced 3He abundance on Solar Orbiter

R. Bučík, G. M. Mason, R. Gómez-Herrero +16

The origin of 3He abundance enhancements in coronal mass ejection (CME)-driven shock gradual solar energetic particle (SEP) events remains largely unexplained. Two mechanisms have…

astro-ph.SR2022★ 29 cited

Evidence of a complex structure within the 2013 August 19 coronal mass ejection. Radial and longitudinal evolution in the inner heliosphere

L. Rodríguez-García, T. Nieves-Chinchilla, R. Gómez-Herrero +9

Context: Late on 2013 August 19, a coronal mass ejection (CME) erupted from an active region located near the far-side central meridian from Earth's perspective. The event and its…

astro-ph.SR2021★ 23 cited

The Long Period of 3He-rich Solar Energetic Particles Measured by Solar Orbiter on 2020 November 17-23

R. Bucik, G. M. Mason, R. Gomez-Herrero +31

We report observations of a relatively long period of 3He-rich solar energetic particles (SEPs) measured by Solar Orbiter. The period consists of several well-resolved ion injectio…

astro-ph.SR2021★ 69 cited

First year of energetic particle measurements in the inner heliosphere with Solar Orbiter's Energetic Particle Detector

R. F. Wimmer-Schweingruber, N. Janitzek, D. Pacheco +45

Solar Orbiter strives to unveil how the Sun controls and shapes the heliosphere and fills it with energetic particle radiation. To this end, its Energetic Particle Detector (EPD) h…

astro-ph.SR2021★ 21 cited

Radial Evolution of the April 2020 Stealth Coronal Mass Ejection between 0.8 and 1 AU -- A Comparison of Forbush Decreases at Solar Orbiter and Earth

Johan L. Freiherr von Forstner, Mateja Dumbović, Christian Möstl +40

Aims. We present observations of the first coronal mass ejection (CME) observed at the Solar Orbiter spacecraft on April 19, 2020, and the associated Forbush decrease (FD) measured…

astro-ph.IM2017★ 8 cited

The Solar Orbiter Mission: an Energetic Particle Perspective

R. Gómez-Herrero, J. Rodríguez-Pacheco, R. F. Wimmer-Schweingruber +27

Solar Orbiter is a joint ESA-NASA mission planed for launch in October 2018. The science payload includes remote-sensing and in-situ instrumentation designed with the primary goal…

astro-ph.SR2013★ 28 cited

Observable effects of Interplanetary Coronal Mass Ejections on ground level neutron monitor counting rates

J. J. Blanco, E. Catalán, M. A. Hidalgo +3

In this work, non-recurrent Forbush decreases (FDs) triggered by the passage of shock-driven interplanetary coronal mass ejections (ICMEs) have been analyzed. Fifty-nine ICMEs have…