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AbstractAbstract
[en] Processes visible during several impulses of new sunspot formations at the periphery of an older large background magnetic field body in which one rotation earlier the large June-July 1974 proton-flare region developed are discussed. The coalescence of separate nuclei into the future umbra and the counter-clockwise rotation of the whole leading region, the change in the sense of rotation during its further development as well as the non-simultaneous development of individual parts of the active region are pointed out. (author)
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Journal Article
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Bulletin of the Astronomical Institutes of Czechoslovakia; ISSN 0004-6248; ; v. 35(4); p. 224-232
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