A new method of forecasting geomagnetic activity and proton showers

Details A new method of forecasting geomagnetic activity and proton showers A new method of forecasting geomagnetic activity and proton showers

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987p%26ss...35..487h&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 35, April 1987, p. 487-491.

Astronomy and Astrophysics

Astronomy

14

Cosmic Ray Showers, Geomagnetism, Magnetic Storms, Prediction Analysis Techniques, Radio Observation, Solar Protons, Heliosphere, Magnetoactivity, Plasma Density, Radio Sources (Astronomy), Solar Terrestrial Interactions

Scientific paper

New ground-based techniques for mapping and tracking large-scale variations of plasma density in the solar wind have shown that disturbances responsible for geomagnetic storms and proton showers may be detected at a distance of 0.6 a.u. from the sun. Continuous observations made during 1978-1979 indicate that the application of this method should lead to substantial improvements in the reliability, and lead-time, of forecasts of geomagnetic activity.

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