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Magnetic observations at the time of the 23 October 1976 solar eclipse in Australia
Affiliation:1. Department of Actuarial Science, Cass Business School, City, University of London, London, UK;2. Department of Finance and Insurance, Faculty of Business, Lingnan University, Hong Kong, China;3. School of Finance, Shanghai University of Finance and Economics, Shanghai, China;1. Department of Internet of Things, East China Jiaotong University, NanChang 330013, PR China;2. School of Computer Science, Guangzhou University, Guangzhou 510631, PR China;3. State Key Laboratory for Novel Software Technology, Nanjing University, Nanjing 210023, PR China
Abstract:The solar eclipse of 23 October 1976 passed across south-east Australia in the local solar afternoon. This paper records the magnetic observations of a line of ten temporary stations stretching from a region of fifty percent obscuration to the path of totality. Magnetic conditions at the time were mildly disturbed. Analyses of the data have sought an eclipse effect in the basic quiet daily variation, and also in the disturbance variations. However, no eclipse effect in the primary ionospheric currents has been clearly distinguished above spatial uneveness, due to local differential induction, in the induced secondary currents flowing in the earth.
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