Abstract
The probability P of overhead occurrence of aurora during a night is estimated for 22 southern hemisphere stations during the I.G.Y. The distribution of probability of occurrence is represented in terms of three measures of colatitude: 81 is defined in terms of the eccentric dipole representation of the geomagnetic field; 82 is defined in terms of projections from circles in the equatorial plane, along the geomagnetic lines of force, onto the Earth; 83 is defined in terms of the integral invariant f; (I-F IF m)!dl of charged particle motion in the geomagnetic field.
Subject
General Physics and Astronomy
Cited by
22 articles.
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1. Candidate Auroral Observations Indicating a Major Solar–Terrestrial Storm in 1680: Implication for Space Weather Events during the Maunder Minimum;The Astrophysical Journal;2021-03-01
2. Long-Term Aspects of Magnetospheric Variability;Physics of Solar Planetary Environments: Proceedings Of the International Symposium on Solar-Terrestrial Physics, June 7-18,1976 Boulder, Colorado Volume II;2013-03-22
3. Characteristic Variations in the Antarctic Ionosphere;Geomagnetism and Aeronomy: Studies in the Ionosphere, Geomagnetism and Atmospheric Radio Noise;2013-03-14
4. Optical observations of gravity waves in the auroral zone;Journal of Atmospheric and Terrestrial Physics;1994-04
5. Auroral electrojet effect on the global occurrence pattern of large scale travelling ionospheric disturbances;Planetary and Space Science;1991-08