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Modeling polar region atmospheric ionization induced by the giant solar storm on 20 January 2005
Author(s) -
Mitthumsiri W.,
Seripienlert A.,
Tortermpun U.,
Mangeard P.S.,
Sáiz A.,
Ruffolo D.,
Macatangay R.
Publication year - 2017
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2017ja024125
Subject(s) - cosmic ray , atmospheric sciences , atmosphere (unit) , ionization , polar , environmental science , solar energetic particles , physics , altitude (triangle) , storm , ionosphere , meteorology , ion , astronomy , coronal mass ejection , plasma , solar wind , nuclear physics , quantum mechanics , geometry , mathematics
Ionization in Earth's troposphere is mainly due to Galactic cosmic rays. Occasionally, solar storms produce intense relativistic ion beams that significantly increase such ionization. One of the largest recorded solar radiation storms, on 20 January 2005, resulted in up to 55‐fold increases in the count rates of ground‐based particle detectors in polar regions. We use McMurdo and Inuvik neutron monitor data to estimate accurate time profiles of ion energy spectra above the atmosphere at each location. Using data‐driven atmospheric models, we perform Monte Carlo simulations of particle‐air interactions and calculate atmospheric ionization and potential biological dosage versus altitude and time for each location. We found that if airplane passengers had traversed the south polar region, they could have been exposed to the typical annual cosmic radiation dosage at sea level within 1 h. These techniques can help evaluate possible influences of solar activity on atmospheric properties.