By Christopher T. Russell (auth.), D. Edgar Page (eds.)
The 1969 ESLAB symposium 'Intercorrelated satellite tv for pc Observations concerning sun occasions' was once held at a time while the significance of bringing jointly degree ments made concurrently in several areas of area used to be starting to be liked. To-day it's universally authorised that the key experimental steps ahead in knowing the physics of the Sun-Earth relationships usually are made via pre-planned correlated satellite tv for pc reviews. Such issues have resulted in the corporation of the foreign Magnetospheric research and the joint ESROj NASA foreign Magnetospheric Explorer, (Mother-Daughter-Heliocentric) venture. The 7th ESLAB symposium was once deliberate as a stick with as much as that of 1969 with the purpose of deriving greatest take advantage of these spacecraft which via luck discovered themselves concurrently working in numerous areas of the magnetosphere and interplanetary area. ESRO had introduced in early 1972 its HEOS-2 satellite tv for pc to enquire fields and debris within the unexplored quarter a long way above the North pole of the Earth and it turned transparent that the fascinating new effects returning from that challenge might profitably be associated with these from quite a few American and the U.S.S.R. PROGNOZ satellites. The booklet follows the order of the symposium (unfortunately the PROGNOZ contribution didn't materialise) concentrating, via either evaluate lectures and of recent experimental effects, at the nature of the bounds among the presentation the interplanetary medium and the magnetosphere and the interplay of every quarter at the other.
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Extra resources for Correlated Interplanetary and Magnetospheric Observations: Proceedings of the Seventh ESLAB Symposium Held at Saulgau, W. Germany, 22–25 May, 1973
I o (\I VO'O I Y o '-' o z 1110 11 20 11 30 UNI VE R S AL 11 40 TIME Fig. 17. One second averages of the vector magnetic field at ATS I and OGO 5 in solar magnetospheric coordinates and the total field strength at the two spacecraft during an isolated substorm on August 7, 1968. At this time OGO and ATS were both close to the midnight meridian. , 1973b). tail. 3 mV m- 1 . Such compressions of the field are not rare in this region, but such an alignment of ATS and OGO during one is. Walker and Kivelson (1972) have reported more than 10 occurrences of such events near midnight in the OGO-5 data, many of them associated with betatron acceleration of electrons and the subsequent generation of ELF chorus emissions.
The principal contribution to the AE index was the integrated southward magnetic field over the previous hour. In this integral northward fields are set equal to zero. Garrett (1973b) has performed a similar study and found two populations of substorms: one set which responds as Arnoldy predicted and one set which responded roughly twice as strongly to an equivalent southward magnetic field, but which was associated with a large variance in the interplanetary magnetic field. , the east-west electric field, integrated over the previous hour controls, the AE index, and the apparent correlation with the variance is due to an association of large variances with high speed streams.
Geophys. Res. 71, 965. Ching, B. K. and Chiu, Y. : 1972a, Planetary Space Sci. 20, 1745. Ching, B. K. and Chiu, Y. : 1972b, Planetary Space Sci. 20,1761. Coleman, P. , Jr. and Smith, E. : 1966, J. Geophys. Res. 71, 4685. Cook, G. : 1968, Planetary Space Sci. 16, 1161. Cook, G. : 1970, Planetary Space Sci. 18, 1573. Coroniti, F. V. and Kennel, C. : 1973, J. Geophys. Res. 78, 2837. Cortie, A. : 1972, Monthly Notices Roy. Astron. Soc. 73, 52. Cummings, W. D. , P. : 1968, Radio Sci. 3, 758. Davis, T.
Correlated Interplanetary and Magnetospheric Observations: Proceedings of the Seventh ESLAB Symposium Held at Saulgau, W. Germany, 22–25 May, 1973 by Christopher T. Russell (auth.), D. Edgar Page (eds.)