On changes in atmospheric circulation after the entry of the earth into a solar corpuscular system

Details On changes in atmospheric circulation after the entry of the earth into a solar corpuscular system On changes in atmospheric circulation after the entry of the earth into a solar corpuscular system

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sva....26..457m&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, July-Aug. 1982, p. 750-762) Soviet Astronomy (ISSN 0038-5301), vol. 26, July-Aug. 1982, p. 4

Astronomy and Astrophysics

Astronomy

1

Atmospheric Circulation, Geomagnetism, Magnetic Storms, Solar Corpuscular Radiation, Solar Terrestrial Interactions, Northern Hemisphere, Pressure Distribution

Scientific paper

Changes in the surface pressure field of the earth above its northern hemisphere after the maxima of sufficiently strong and relatively isolated geomagnetic storms are studied in the present article, based on daily weather maps for the period of 1880-1974. It is found that the maximum increase in atmospheric instability after geomagnetic storms takes place mainly above oceans, especially in regions where cool and warm currents come together, as well as near the 'ocean-land' boundary. Moreover, the entry of the earth into a corpuscular stream is accompanied by pronounced deepening of the Icelandic and Aleutian lows, and almost simultaneously by a pressure increase over Europe and Alaska. All these effects are clearest in the cold period of the year and especially in those cases when the corpuscular stream under consideration is not preceded by another stream close to it (the role of the initial conditions).

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