Anomalous N(h) profiles in the high-latitude ionosphere

Details Anomalous N(h) profiles in the high-latitude ionosphere Anomalous N(h) profiles in the high-latitude ionosphere

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..849b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, Sept.-Oct. 1986, p. 849, 850. In Russian.

Physics

1

Auroral Ionization, E Region, F 2 Region, Ionospheric Ion Density, Anomalies, Atmospheric Models, Kp Index, Polar Substorms

Scientific paper

It is shown that empirical models of NmF2 and anomalous density in the E region can be used to define the conditions for the formation of anomalous N(h) profiles in the auroral oval under different solar and geophysical conditions. To illustrate this, NmE and NmF2 ratios corresponding to solar maximum and minimum epochs for Kp = 0-1 and Kp = 3-4 (the development of substorm activity) were calculated for 00, 06, 12, and 18 h UT, December 1958 and 1964.

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