Monitoring of heliosphere, magnetosphere and atmosphere via cosmic ray effects in August 2018

I. I. Kovalev; Ковалев И. И.; S. V. Olemskoy; Олемской С. В.; V. E. Sdobnov; Сдобнов В. Е.; A. N. Dmitrieva; Дмитриева А. Н.; V. V. Shutenko; Шутенко В. В.

doi:10.31857/S036767652370182X

Monitoring of heliosphere, magnetosphere and atmosphere via cosmic ray effects in August 2018

Авторлар: Kovalev I.I.¹, Olemskoy S.V.¹, Sdobnov V.E.¹, Dmitrieva A.N.², Shutenko V.V.²
Мекемелер:
1. Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences
2. National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Шығарылым: Том 87, № 7 (2023)
Беттер: 1028-1031
Бөлім: Articles
URL: https://edgccjournal.org/0367-6765/article/view/654361
DOI: https://doi.org/10.31857/S036767652370182X
EDN: https://elibrary.ru/OSNWXJ
ID: 654361

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Аннотация
Авторлар туралы
Әдебиет тізімі
Қосымша файлдар
Статистика

Аннотация

Using data of ground-level cosmic ray measurements on the neutron monitor network, along with data of Yakutsk muon telescope complex and muon hodoscope URAGAN (Moscow) uncorrected for temperature, we used modified spectrographic global survey method for an August 2018 event to split cosmic ray variations into components of primary, magnetospheric and atmospheric origin. Time evolutions of isotropic primary flux for different rigidities, pitch-angle anisotropy of cosmic rays, interplanetary magnetic field orientation were obtained, variations in geomagnetic cut-off rigidity in Irkutsk and average-mass temperature over charged components’ measurement sites were also shown.

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