By Juan G. Roederer (auth.), K. Knott, B. Battrick (eds.)
ISBN-10: 9401018928
ISBN-13: 9789401018920
ISBN-10: 9401018944
ISBN-13: 9789401018944
The tenth ESLAB Symposium was once held at Grossenzersdorf close to Vienna on 10-13 June 1975 less than the name 'The clinical satellite tv for pc Programme in the course of the Inter nationwide Magnetospheric Study'. The Symposium was once attended via an invited viewers of 60 scientists from the ESA Member States, the us, Japan, Canada and Austria. Following a document via the joint COSPAR-IUCSTP precise operating crew, the overseas Magnetospheric examine (lMS) is proposed as a global co operative company of restricted length, having as its important aim the achie vement of a entire, quantitative realizing of the dynamical procedures working within the Earth's plasma and box atmosphere. with a purpose to accomplish this goal, it truly is regarded as essential to perform simultaneous measurements with approximately exact instrumentation at quite a few issues in area. those measurements might want to be made together with applicable observations at or close to the Earth's floor. in addition to near-Earth observations by way of ground-based, rocket- and balloon-borne instrumentation, satellite tv for pc investigations are anticipated to make a huge contri bution to the IMS. a couple of satellites assigned to magnetospheric learn have lately been introduced, or may be introduced presently, to be operational throughout the IMS. the eu house employer has dedicated of its imminent clinical satellites - GEOS and ISEE-B - to magnetospheric and interplanetary research.
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Additional info for The Scientific Satellite Programme during the International Magnetospheric Study: Proceedings of the 10th ESLAB Symposium, Held at Vienna, Austria, 10–13 June 1975
Example text
The asymmetries in these flows have been shown by Heppner [1972] to be controlled by the direction of the dawndusk component of the interplanetary magnetic field. However, we do not yet have a quantitative correlation between the potential drop across the polar cap and interplanetary conditions, nor do we know how to relate the size of the asymmetry to the magnitude of the dawn-ta-dusk interplanetary magnetic fields. , 1973]. , 1973]. These currents are often accompanied by VLF electrostatic waves which in turn can cause anomalous resistivity leading to potential drops which are able to accelerate particles to auroral energies.
127622. 8140. 1 VELAs may be operated during some IMS periods Remarks Solar pointed & wheel expts. Some geocoronai expts. SOLRAD IIA II/ /75 o. SOLRAD liB II/ /75 o. P78-1 /78 IQ/ Period (min) Sci. type S 0 L A R Launched with Solwind expt. 0 SESP 74-2 IQ/ /76 90. 200. 8000. GEOS 02/ /77 I. 35700. 35700. ISEE-A &-B 10/ /77 28. 280. 133852. 3270. EXOS-B 08/ /78 30. 500. 30000. 480. 2 Only synchronous SIC dedicated to IMS. 25'W-35'E-O'E-35'E long. 5 D5-B 05/25/75 SESP 73-6 3QI /75 90. 230. 900. AE-D 091 /75 98.
80, in press, 197 5. , The structure of the exosphere or adventures in velocity space, in Geophysics, The Earth's Environment, (Eds. C. DeWitt, J. Hieblot & A. Lebeau), Gordon and Breach, New York, 1963. , The length of the magnetospheric tail, 1. Geophys. Res. 70(7), 1753 (1965). , Present status of the ISEE A and B Mission, Proc. 10th ESLAB Symposium, this volume, 1975. , Personal communication, 1975. T. D. Means, F. Scarf & M. Neugebauer, The perpendicular bow shock, in preparation, 197 Sa. T.
The Scientific Satellite Programme during the International Magnetospheric Study: Proceedings of the 10th ESLAB Symposium, Held at Vienna, Austria, 10–13 June 1975 by Juan G. Roederer (auth.), K. Knott, B. Battrick (eds.)
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