Direct Measurements of Synchrotron-emitting Electrons at Near-Sun Shocks

Abstract In this study, we present the first-ever direct measurements of synchrotron-emitting heliospheric traveling shocks, intercepted by the Parker Solar Probe (PSP) during its close encounters. Given that much of our understanding of powerful astrophysical shocks is derived from synchrotron radiation, these observations by PSP provide an unprecedented opportunity to explore how shocks accelerate relativistic electrons and the conditions under which they emit radiation. The probe’s unparalleled capabilities to measure both electromagnetic fields and energetic particles with high precision in the near-Sun environment has allowed us to directly correlate the distribution of relativistic electrons with the resulting photon emissions. Our findings reveal that strong quasi-parallel shocks emit radiation at significantly higher intensities than quasi-perpendicular shocks due to the efficient acceleration of ultrarelativistic electrons. These experimental results are consistent with theory and recent observations of supernova remnant shocks and advance our understanding of shock physics across diverse space environments.

Authors

Institutions

Publication Details

Journal
The Astrophysical Journal Letters
Published
2024-11-01
DOI
https://doi.org/10.3847/2041-8213/ad8eb8
Citations
11
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
3.65
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Direct Measurements of Synchrotron-emitting Electrons at Near-Sun Shocks

N. E. Raouafi, Lucas Colomban, N. Dresing, М. А. Балихин et al.
11 citations
The Astrophysical Journal Letters
Solar and Space Plasma Dynamics
3.65
article

Direct Measurements of Synchrotron-emitting Electrons at Near-Sun Shocks

N. E. Raouafi, Lucas Colomban, N. Dresing, М. А. Балихин, I. C. Jebaraj, F. S. Mozer, O. V. Agapitov, Erika Palmerio, Anastasiia Marmyleva, M. Gedalin, D. J. McComas, M. Pulupa, L. Vuorinen, Nicolas Wijsen, Andrii Voshchepynets, V. Krasnoselskikh, M. Miceli, Rami Vainio, Jens Pomoell, Athanasios Kouloumvakos
article en
11 citations

Abstract

Abstract In this study, we present the first-ever direct measurements of synchrotron-emitting heliospheric traveling shocks, intercepted by the Parker Solar Probe (PSP) during its close encounters. Given that much of our understanding of powerful astrophysical shocks is derived from synchrotron radiation, these observations by PSP provide an unprecedented opportunity to explore how shocks accelerate relativistic electrons and the conditions under which they emit radiation. The probe’s unparalleled capabilities to measure both electromagnetic fields and energetic particles with high precision in the near-Sun environment has allowed us to directly correlate the distribution of relativistic electrons with the resulting photon emissions. Our findings reveal that strong quasi-parallel shocks emit radiation at significantly higher intensities than quasi-perpendicular shocks due to the efficient acceleration of ultrarelativistic electrons. These experimental results are consistent with theory and recent observations of supernova remnant shocks and advance our understanding of shock physics across diverse space environments.

The Astrophysical Journal LettersVol. 976(1)
Centre National de la Recherche Scientifique (FR), Laboratoire de Physique et Chimie de l’Environnement et de l’Espace (FR)
Openalex Percentile: Top 7%
Solar and Space Plasma Dynamics
3.65
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.