Abstract
A3 measurements on 2.83 MHz over a distance of 502 km of some 17 months are analyzed. The results are sorted by solar zenith angles, asymmetries derived and a relation to the sunspot number sought. It is furthermore attempted to include night absorption in the analysis. Some of the possible systematic errors are qualitatively described.
Originalsprache | englisch |
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Seiten (von - bis) | 155-161 |
Fachzeitschrift | Kleinheubacher Berichte |
Jahrgang | 21 |
Publikationsstatus | Veröffentlicht - 1978 |