M Region Magnetic Storm

From ExoDictionary
Jump to: navigation, search
This definition page has been automatically generated.
You can help ExoDictionary by expanding, updating, or correcting it.


This autostub has not yet had its initial copyediting proof and may contain significant formatting and even factual errors. You can improve Exodictionary by cleaning up the page markup and verifying that the definition is correct and then removing this tag.


This autostub has not yet had its initial categorization proof and may be categorized incorrectly. You can improve Exodictionary by removing inappropriate categories and then removing this tag.


M Region Magnetic Storm

</dt>
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. </dd>

References

This article is based on NASA's Dictionary of Technical Terms for Aerospace Use