By Kagermann H., Koehler W.
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Geo- 8087-8096. Russell planetary space with time variation rotation period. J. Geophss. L. T. Russell (1975b)' An relationship between interplanetary conditions J. Geoph•,s. , 8__•0, 4204-4214. , Russell observed in Bursts of inter- of the planetary 7__•9,3551-3558. of Mars, in on Cosmochemistry 537 Copyright American Geophysical Union of Physics of Solar Planetary Environments: Proceedings of the International Symposium on Solar-Terrestrial Physics June 7–18,1976, Boulder, Colorado, Volume II Special Publications Dolginov, Sh.
It appears that someof the unusually thick magnbtopause crossings in Hyde's study may have included the boundarylayer thickness as part of the magnetopause. 200• -_qO o 0 Fig. 6. GO 120 180 240 OGO-5magnetometerrecord, March 14, 1968, starting 900 s•cs. at 20:24:00 UT {X = 48130, Y = -20240, Z = 3330 km}. Hodogram basedon data inter- val indicated by shaded horizontal bar is shownin figure 5b. 550 Copyright American Geophysical Union Special Publications Physics of Solar Planetary Environments: Proceedings of the International Symposium on Solar-Terrestrial Physics June 7–18,1976, Boulder, Colorado, Volume II Vol.
Mackin and M. 7-263. , H. D. Montgomery,G. Paschmann,and N. Schopke (1975)' HEOS-2plasmaobservationsin the distant polar magnetosphere' the plasmamantle. J. , 80:2723. Sonnerup, B. U. , andL. J. Cahill, Jr. (1967): Magnetopause structureand attitude from Explorer 12 observations. J. , 72:171. Sonnerup, B. U. , andL. J.