G. Teleki (auth.), W. Fricke, G. Teleki (eds.)'s Sun and Planetary System: Proceedings of the Sixth European PDF

By G. Teleki (auth.), W. Fricke, G. Teleki (eds.)

ISBN-10: 9400978464

ISBN-13: 9789400978461

ISBN-10: 9400978480

ISBN-13: 9789400978485

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Read Online or Download Sun and Planetary System: Proceedings of the Sixth European Regional Meeting in Astronomy, Held in Dubrovnik, Yugoslavia, 19–23 October 1981 PDF

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Extra info for Sun and Planetary System: Proceedings of the Sixth European Regional Meeting in Astronomy, Held in Dubrovnik, Yugoslavia, 19–23 October 1981

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40 961. 31 961. 52 961. 40 961. 28 961. 2 7 961. 40 961. 45 961. 32 961. 27 961. 25 110 142 117 172 170 96 97 67 4 3 4 5 4 3 3 3 1956 1957 1958 1959 1960 1961 1962 1963 1964 1965 1966 1967 1968 1969 1970 1971 961. 41 961. 17 961. 28 961. 56 961. 45 961. 29 961. 36 961. 48 961. 56 961. 48 961. 72 56 112 104 143 135 114 82 59 93 103 83 76 105 115 117 117 961. 61 961. 85 961. 18 961. 18 961. 15 961. 45 60 114 108 142 142 133 77 55 83 104 65 78 100 120 109 118 7 5 5 6 7 8 9 7 9 9 9 9 11 12 10 1975 1976 1977 1978 1979 1980 1981 961.

Solar gamma lines were first observed by Chupp et al. (1973) during the flare of August 4, 1972. KOCHAROV spacecraft (February-December, 1980). , 1981; Simnett, 1981). An analysis of the available data leads to the following conclusions: 1. 16 UT. The width of the individual spikes is qualitatively similar in all sets. The first series lasted about 70 s at the event onset. The number of subpulses in the first series is 7. The modulation depth is typically a factor of 4 during the first series of spikes.

The space era has allowed to slightly improve this situation; on one side, one can measure the energy in the invisible parts of the spectrum, non observable from the ground, IR or XUV ••. ; on the other side, the transparency in the observable parts is not any more affected by· climatological conditions. The results are accordingly much better, and the accuracy of 1% can be reached; strangely enough, this is still considered as a good determination (see table I). The limitation rests now in the spottedness of solar surface.

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Sun and Planetary System: Proceedings of the Sixth European Regional Meeting in Astronomy, Held in Dubrovnik, Yugoslavia, 19–23 October 1981 by G. Teleki (auth.), W. Fricke, G. Teleki (eds.)


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