view Abstract Citations (1) References Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Solar corpuscles responsible for geomagnetic disturbances. Pecker, Jean-Claude ; Roberts, Walter Orr Abstract Some years ago C. W. Allen presented all extensive analysis of geomagnetic storms, and offered suggestions for their explanation in terms of streams of corpuscles originating in the sun.' We offer a qualitative hypothesis, that incorporates Allen's suggestions and identifies the solar source of corpuscular emission responsible both for recurrent and non-recurrent geomagnetic disturbances. We postulate two different types of solar sources of such particles as follows: (a) Small jets of corpuscles, distributed in a fine network all over the surface of the sun, and presumably associated with chromospheric spicules or photospheric granules. These jets, in the absence of deflecting solar magnetic fields, would send radial streams of corpuscles in all directions; the streams would be present at all times, regardless of the state of solar activity. In the presence of deflecting magnetic fields from active centers, and the general magnetic field of the sun, the corpuscles are deflected to form the streams responsible for the recurrent "M-region" geomagnetic disturbances. (b) Irregular streams of ions associated with active regions, and probably most intense at the time of solar flares. Not all active centers have such streams present at all times, and there is probably also a large dispersion of particle velocities and stream energies for this type of corpuscular stream. We present evidence from a study of geomagnetic disturbances in 1952-53 to support the hypothesis of the formation of recurrent magnetic storms by particle streams of the first type. In particular we find evidence that above certain active regions there is a "cone of avoidance" with low particle density. The center of the cone reaches earth three days later. We also show that there is some evidence that at the edges of the cone-of-avoidance the deficiency of corpuscles is compensated by regions with an excess particle density. The hypothesis is in accord with the explanation we gave earlier for the formation of the K component of the white light corona,' here associated with the solar-terrestrial corpuscular beams. The hypothesis suggests that daily coronagraphic observation of the white light corona may prove of great value for prediction of the times of occurrence of geomagnetic storms and associated phenomena. This work was supported by the Air Force Cambridge Research Center, Geophysical Research Directorate, Air Research and Development Command. 5.M. N. 104, 53, 5944. 2.Roberts, W. 0., R. Grenchik, and D. E. Billings, A. f. 58, 225, 5953. High Altitude Observatory, Boulder, Colo. Publication: The Astronomical Journal Pub Date: October 1954 DOI: 10.1086/107040 Bibcode: 1954AJ.....59..330P full text sources ADS |
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