Mid-latitude magnetic bays and auroral absorption

Details Mid-latitude magnetic bays and auroral absorption Mid-latitude magnetic bays and auroral absorption

Sep 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970p%26ss...18.1301l&link_type=abstract

Planetary and Space Science, Volume 18, Issue 9, p. 1301-1306.

Computer Science

Scientific paper

One hundred and thirty two simple isolated magnetic bay events at Fredericksburg, Virginia, were studied in terms of their H, Z and D components and found to fall into several distinct groups. Nighttime bays are sharp, highly correlated with 18 MHz auroral absorption at mid-latitude stations, and their H and Z components reverse sign near 2100 hr LT. Daytime bays are generally diffuse and only slightly correlated with mid-latitude riometer absorption. The high degree of correspondence between sharp bays and riometer absorption suggests that the same precipitating particles may be responsible for both.

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