Volume 444 -
38th International Cosmic Ray Conference (ICRC2023) -
Solar & Heliospheric Physics (SH)
Interplanetary Coronal Mass Ejection of October 3, 2021
Full text:
pdf
Pre-published on:
July 25, 2023
Published on:
—
Abstract
Magnetic clouds are closed structures immersed within interplanetary coronal mass ejections. These structures have an important effect on the propagation of solar energetic particles and cosmic rays that is observed as variations in the flux of these particle populations. On November 3, 2021 one of these structures was observed at different solar distances by instruments aboard Solar Orbiter and instruments in Earth orbit. The topology of the magnetic cloud has been analyzed by observing its evolution between the different observation points and the effect on solar energetic particles and cosmic rays
DOI: https://doi.org/10.22323/1.444.1347
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.
Open Access
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.