M Region Magnetic Storm
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M Region Magnetic Storm
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A magnetic storm that is independent of visible solar disk features; it
begins gradually and shows a strong tendency to recur within a period of 27
days.
</dd>
The hypothetical region on the solar disk assumed to be the source of
the incident corpuscular radiation is called the M-region.
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[edit] References
This article is based on NASA's Dictionary of Technical Terms for Aerospace Use
