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• W1855015909 abstract "The Carte Synoptique catalogue of solar filaments from 1919 March to 1957 July, corresponding to complete cycles 16-18, is utilized to show the latitudinal migrations of solar filaments at low (≤50°) and high (>50°) latitudes and the latitudinal distributions of solar filaments for all solar filaments, solar filaments whose maximum lengths during solar disk passage are less than or equal to 70° and solar filaments whose maximum lengths during solar disk passage are larger than 70°. The results show the following. (1) The latitudinal migrations of all low-latitude solar filaments and low-latitude solar filaments whose maximum lengths during solar disk passage are less than or equal to 70° follow the Spörer sunspot law. However, the latitudinal migration of low-latitude solar filaments whose maximum lengths during solar disk passage are larger than 70° do not follow the Spörer sunspot law: there is no equatorward and no poleward drift. The latitudinal migration of high-latitude solar filaments whose maximum lengths during solar disk passage are larger than 70° is more significant than those of all high-latitude solar filaments and high-latitude solar filaments whose maximum lengths during solar disk passage are less than or equal to 70°: there is a poleward migration from the latitude of about 50° to 70° and an equatorward migration from the latitude of about 70° to 50° of all high-latitude solar filaments and high-latitude solar filaments whose maximum lengths during solar disk passage are less than or equal to 70° and there is a poleward migration from the latitude of about 50° to 80° and an equatorward migration from the latitude of about 80° to 50° of high-latitude solar filaments whose maximum lengths during solar disk passage are larger than 70°. (2) The statistical characteristics of latitudinal distribution of solar filaments whose maximum lengths during solar disk passage are larger than 70° is different from those of all solar filaments and solar filaments whose maximum lengths during solar disk passage are less than or equal to 70° (© 2012 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)" @default.
• W1855015909 created "2016-06-24" @default.
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• W1855015909 date "2012-08-01" @default.
• W1855015909 modified "2023-10-16" @default.
• W1855015909 title "Cyclical behavior of solar filaments" @default.
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• W1855015909 doi "https://doi.org/10.1002/asna.201111693" @default.
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