On the behavior of the Dst geomagnetic index in the vicinity of magnetic cloud passages at Earth

Journal Article · Mon Jan 01 04:00:00 EST 1990 · Journal of Geophysical Research; (United States)

DOI:https://doi.org/10.1029/JA095iA01p00215· OSTI ID:5221394

Wilson, R M ^[1]

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1. NASA Marshall Space Flight Center, Huntsville, AL (United States)

The geomagnetic response to magnetic clouds is investigated for the 34 magnetic clouds observed between 1973 and 1982, in particular, according to cloud type: southward turning clouds as compared to northward turning clouds. While, on average, the most negative Dst value associated with interplanetary magnetic clouds is the one for northward turning clouds, the difference in the depths of decrease (onset Dst value minus the most negative Dst value during cloud passage) for the two cloud types does not appear to be statistically important; hence northward turning and southward turning clouds have depths of decrease (negative excursions in the Dst index) of comparable size, differing primarily in the time of most negative Dst occurrence (relative to cloud onset at Earth). For northward turning clouds, the most negative Dst value usually occurs within 12 hours of cloud onset at Earth, while for southward turning clouds it is delayed until after 12 hours from cloud onset. Such behavior is consequential in that it is directly related to the occurrence of southward Bz.

• OSTI ID: 5221394
• Journal Information: Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 95:A1; ISSN 0148-0227; ISSN JGREA
• Country of Publication: United States
• Language: English

Related Subjects

640201* -- Atmospheric Physics-- Auroral
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
EARTH ATMOSPHERE
EARTH MAGNETOSPHERE
FUNCTIONS
GEOMAGNETIC FIELD
INTERACTIONS
INTERPLANETARY SPACE
MAGNETIC FIELDS
MAGNETIC STORMS
MASS TRANSFER
RESPONSE FUNCTIONS
SOLAR ACTIVITY
SOLAR WIND
SPACE
VELOCITY