NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Correlations of OGO-V plasmapause crossing with observations of type Pi micropulsations on the ground.Comparison of plasmapause positions with Pi micropulsation events observed at College (L 5.4) or at Sodankyla (L 5.1), showing that in almost all cases the plasmapause was inside the field line of the observing site when the Pi event was recorded. Strong Pi events were seen at Nurmijaarvi (L 3.4) only when Kp was very high, when the plasmapause would be expected to be inside L 3.4. When Pi events and structure Pc 1 events were observed nearly simultaneously, the Pi activity was always more prominent at the poleward site. A demarcation line seems to exist, separating the Pi and structured Pc 1 source regions. This line may be the plasmapause, with structured Pc 1 inside and Pi outside.
Document ID
19720037557
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Heacock, R. R.
Mullen, A. J.
Hessler, V. P.
(Alaska, University College, Alaska, United States)
Sucksdorff, C.
Kivinen, M.
(Finnish Meteorological Institute Helsinki, Finland)
Kataja, E.
(Sodankyla Geophysical Observatory Sodankyla, Finland)
Date Acquired
August 6, 2013
Publication Date
December 1, 1971
Publication Information
Publication: Annales de Geophysique
Volume: 27
Subject Category
Geophysics
Report/Patent Number
NSSDC-ID-68-014A-14-OM
Accession Number
72A21223
Funding Number(s)
CONTRACT_GRANT: NAS5-9092
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available