Anisotropic Forbush decrease of 24 March 2024: First look
Mishev, Alexander; Larsen, Nicholas; Asvestari, Eleanna; Sáiz, Alejandro; Ann Shea, Margaret; Strauss, Du Toit; Ruffolo, David; Banglieng, Chanoknan; Seunarine, Surujhdeo; Duldig, Marc L.; Gil, Agnieszka; Blanco, Juan José; García-Población, Oscar; Cervino-Solana, Pablo; Adams,, James H.; Usoskin, Ilya (2024-08-14)
Mishev, Alexander
Larsen, Nicholas
Asvestari, Eleanna
Sáiz, Alejandro
Ann Shea, Margaret
Strauss, Du Toit
Ruffolo, David
Banglieng, Chanoknan
Seunarine, Surujhdeo
Duldig, Marc L.
Gil, Agnieszka
Blanco, Juan José
García-Población, Oscar
Cervino-Solana, Pablo
Adams,, James H.
Usoskin, Ilya
Elsevier
14.08.2024
Alexander Mishev, Nicholas Larsen, Eleanna Asvestari, Alejandro Sáiz, Margaret Ann Shea, Du Toit Strauss, David Ruffolo, Chanoknan Banglieng, Surujhdeo Seunarine, Marc L. Duldig, Agnieszka Gil, Juan José Blanco, Oscar García-Población, Pablo Cervino-Solana, James H. Adams, Jr., Ilya Usoskin, Anisotropic Forbush decrease of 24 March 2024: First look, Advances in Space Research, Volume 74, Issue 8, 2024, Pages 4160-4172, ISSN 0273-1177, https://doi.org/10.1016/j.asr.2024.08.027
https://creativecommons.org/licenses/by/4.0/
© 2024 COSPAR. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
https://creativecommons.org/licenses/by/4.0/
© 2024 COSPAR. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
https://creativecommons.org/licenses/by/4.0/
Julkaisun pysyvä osoite on
https://urn.fi/URN:NBN:fi:oulu-202409025672
https://urn.fi/URN:NBN:fi:oulu-202409025672
Tiivistelmä
Abstract
A strong Forbush decrease, i.e., suppression of the flux of galactic cosmic rays recorded on Earth, was observed by the global network of ground-based neutron monitors (NMs) on 24 – 25 March 2024. The decrease was very unusual as characterised by so rapid recovery that a false Ground-level enhancement (GLE) alarm was produced by the corresponding warning systems. Here we present the first comprehensive collection and analysis of the available data for this event. The event was highly anisotropic as exhibited in a 3-h spread of the deep-phase timing for different NMs. The anisotropy was focused nearly at the anti-sunward direction with a narrow cone of 20 – 30°. The heliospheric situation leading to this unusual Forbush decrease was quite complex. An analysis of first look records was performed, considering the stations acceptance, taking into account the complex geomagnetic conditions. A leader fraction analysis indicates that the recovery phase of the event was rigidity-independent and had essentially the same spectral shape as the pre-event period. A summary of the solar-terrestrial phenomena is provided to assist in future work on modelling this complex event.
A strong Forbush decrease, i.e., suppression of the flux of galactic cosmic rays recorded on Earth, was observed by the global network of ground-based neutron monitors (NMs) on 24 – 25 March 2024. The decrease was very unusual as characterised by so rapid recovery that a false Ground-level enhancement (GLE) alarm was produced by the corresponding warning systems. Here we present the first comprehensive collection and analysis of the available data for this event. The event was highly anisotropic as exhibited in a 3-h spread of the deep-phase timing for different NMs. The anisotropy was focused nearly at the anti-sunward direction with a narrow cone of 20 – 30°. The heliospheric situation leading to this unusual Forbush decrease was quite complex. An analysis of first look records was performed, considering the stations acceptance, taking into account the complex geomagnetic conditions. A leader fraction analysis indicates that the recovery phase of the event was rigidity-independent and had essentially the same spectral shape as the pre-event period. A summary of the solar-terrestrial phenomena is provided to assist in future work on modelling this complex event.
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