By K. Knott (auth.), K. Knott, A. Durney, K. Ogilvie (eds.)

(Opening handle of thirteenth ESLAB Symposium) With GEOS and ISEE occupying a massive a part of the ESA medical programme it used to be transparent a number of years in the past 'natural' foundation for the 1978 ESLAB Annual Symposium often is the early facts from those spacecraft. throughout the 1976 assembly of the eu Geophysical Society in Amsterdam it turned obvious to me a lot wider group used to be and that during specific operating workforce 2 of COSPAR used to be contemplating a GEOS consultation in the course of its 1978 assembly right here in Innsbruck. This was once after all because it should be simply because GEOS were followed because the reference spacecraft for the foreign Magnetospheric examine. After a few discussions with COSPAR and with the organizers of the STP Symposium which was once held the following final week we felt that during the curiosity of shopper kinfolk and following strong good judgment we should always hand over a few of our independence in 1978 and merge our Symposium with COSPAR. i'd gratefully recognize the co-operation of COSPAR's operating workforce 2 chairman and vice-chairman, the energetic aid of the President of COSPAR and the 'gentleman's contract' with the STP programme committee which prepared that the hot ISEE and GEOS effects have been routed to this Symposium instead of to the STP. i've got noted how we got here to have this joint Symposium. maybe I may still let you know too how we got here as regards to having no Symposium.

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Since a long time intensive studies of Pc-1-Pi-1 have been carried out using ground data, and a classification of the different types of events which can be observed in this frequency range has been made based on their spectral shapes on Space Science Reviews :u (1978) 347-369. All Rights Reserved Copyright © 1978 by D. Reidel Publishing Company, DortlTecht, Holland 27 348 s. PERRAUT ET AL. a three dimensional representation (Gendrin, 1970). Generally these pulsations observed on ground have frequencies below the minimum proton gyrofrequency along the field line and they are left hand polarized.

KILAUT In' AL The conditions of generation of the harmonically related structures have not been studied in enough details. In particular, it would be interesting to have more measurements about the angular distribution of protons at energies below 20 )reV. Similarly we should verify if these emissions are restricted to a well defined region around the geomagnetic equator as evidenced by Gurnett (1976) for low Lvalues. , 1978). We are grateful to Dr P. Decreau (Centre de Recherc:he en Physique de l~ Issy MouHneaux, France), to Dr A.

FargcttoD. , and LaaJume, J. , Space Sd.. Rev. Z2, 433. Gumett. D. A: 1976. J. Geophya. Res. 8~ 2765. Heppner, J. , Sugiura, M, ~1man. T. L. Ledley, B. : 1967,1. Geophy•. Res. n, 5417. Heppner, J. , Ledley, B. , Skillman, T. s and Sugium. M: 1970, Ann. Gtophy£. 26, 709. Hughes, W. J.. • and Barfield. I. : 1978, 1. Geophys. Res. Ill, 1109. : 1978, Space Sci. Reu.. Z%. 327. Kennel, C. , Scmf. F. , Fredricks. R. , McGhee, J. , and Coroniti, F. : 1970, J. Gvophys. Res. 75, 6136. Kintner, P. M. and Gumett.

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Advances in Magnetosperic Physics with GEOS-1 and ISEE by K. Knott (auth.), K. Knott, A. Durney, K. Ogilvie (eds.)
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