Comparison of Atmospheric Ionization for Solar Proton Events of the Last Three Solar Cycles

被引：1

作者：

Maurchev, Eugene A. ^{[1
]}

Shlyk, Nataly S. ^{[1
]}

Dmitriev, Alexey V. ^{[2
]}

Abunina, Maria A. ^{[1
]}

Didenko, Kseniia A. ^{[1
]}

Abunin, Artem A. ^{[1
]}

Belov, Anatoly V. ^{[1
]}

机构：

[1] Russian Acad Sci IZMIRAN, Pushkov Inst Terr Magnetism Ionosphere & Radio Wav, Kaluzhskoe hw 4, Troitsk 108840, Moscow, Russia

[2] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Leninskie Gory 1-2, Moscow 119899, Russia

来源：

ATMOSPHERE | 2024年 / 15卷 / 02期

关键词：

atmospheric ionization; solar energetic particles; ground-level enhancements; GROUND-LEVEL ENHANCEMENT; STATISTICAL-ANALYSIS; ENERGETIC PARTICLES; MODEL; FLARES; EJECTIONS; GLE;

D O I：

10.3390/atmos15020151

中图分类号：

X [环境科学、安全科学];

学科分类号：

08 ; 0830 ;

摘要：

Numerical modeling of primary cosmic ray protons' transport through the Earth's atmosphere was performed for the energy spectra of solar energetic particle events (SEPs). Several events in the last three solar cycles were considered. A comparative analysis of the characteristics of coronal mass ejections and primary proton fluxes was carried out. The main results were quantitative estimates of the calculated atmospheric ionization count rate for a wide range of altitudes (from sea level up to 98 km). The difference in the influence of solar protons on the Earth's atmosphere is considered for seven SEPs divided into three groups with similar solar sources (X-flare magnitude and coordinates) but with different characteristics of accelerated particle fluxes. The data obtained in this work are very important for future studies of radio wave propagation, atmospheric chemistry and climate change.

引用

页数：15

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