Other
Scientific paper
Mar 1958
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1958natur.181..641t&link_type=abstract
Nature, Volume 181, Issue 4609, pp. 641-642 (1958).
Other
Scientific paper
FROM observations of magnetic disturbances on the Earth, Bartels1 suggested the existence of M-regions on the Sun. Attempts have been made to associate these M-regions with other solar phenomena. Allen2 tried to show that coronal streams and M-regions are identical; he also concluded that M-regions avoid spot groups or are even destroyed by them. This conclusion was implicitly modified by the results of Denisse3 and Becker4. Identification of M-regions with regions of unusually weak corona emission was recently suggested by Bell and Glazer5. Kiepenheuer6 arrived at the conclusion that filaments are the possible source of M-disturbances. As a result of measurements of the solar magnetic field, Babcock and Babcock7 believed that the observed unipolar magnetic regions are M-regions. With these measurements M-regions may have ceased to be hypothetical in character. Whether or not this is so, it is still of interest to continue the study of M-regions relative to other solar phenomena.
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