Lv. Egorova et al., Influence of variations of the cosmic rays on atmospheric pressure and temperature in the Southern geomagnetic pole region, J ATMOS S-P, 62(11), 2000, pp. 955-966
Citations number
24
Categorie Soggetti
Earth Sciences
Journal title
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS
Daily data of pressure, temperature, and wind observations at Antarctic sta
tion Vostok in 1981-1991 have been analyzed with regard to the cosmic-rays
variations. Case study and statistical treatment of the data provide the fo
llowing results. The beginning of the Forbush decrease of galactic cosmic r
ays is followed within one day by significant warming of the atmosphere (ab
out 10 degrees) at altitudes h < 6-7 km in the near-pole region. The durati
on of warming is about 1 day, then the atmosphere quickly reverted to previ
ous temperature conditions. The Forbush decrease is accompanied by reductio
n of atmospheric pressure at all altitudes below 20 km, the magnitude of re
duction being maximal at higher altitudes. The reduction of atmospheric pre
ssure can develop synchronously with the Forbush decrease or can be delayed
for 1-5 days depending on the preceding trends in the meteorological proce
sses, occurrence of the solar proton spikes, and intensity of the Forbush d
ecrease. Spikes of solar cosmic rays affect within 0-2 days the increase of
atmospheric pressure at altitudes of 10-15 km. The troposphere warming and
reduction of the pressure in low stratosphere and troposphere is followed
within 0-6 days by reconstruction of the whole wind system above the near-p
ole region. (C) 2000 Elsevier Science Ltd. All rights reserved.