责怪
发表于 2025-3-23 13:09:59
1743-9213 problems were stressed and the majority of the Scientific Organizing Committee agreed not to deal with short-lived phenomena of the solar activity or with indiv978-90-277-0681-2978-94-010-1481-6Series ISSN 1743-9213 Series E-ISSN 2352-2186
豪华
发表于 2025-3-23 15:41:27
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objection
发表于 2025-3-23 21:02:48
Heritagization of the Camino to Finisterre solar differential rotation and to search for giant cell circulation pattern. Details of the observing method and the results from observations during 1974 have been published very recently (Schröter and Wöhl, 1975). Our method consists of measuring the position of 5–15 bright Ca.-mottles with res
B-cell
发表于 2025-3-24 01:30:25
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粘连
发表于 2025-3-24 03:11:58
Kai Maaz,Marko Neumann,Jürgen Baumertore than 15 years of observations are given. The major part of our information concerns the morphology and only some results deal with the kinematics of the field distribution. Results of averaged solar magnetic field fluxes and polarity reversal studies as well as of preliminary investigation of th
离开
发表于 2025-3-24 09:10:07
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Antioxidant
发表于 2025-3-24 13:08:33
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blithe
发表于 2025-3-24 18:23:02
Herman Heijermans and His Dramasund between the maximum values of the limb effect of the redshift, the boundaries of polarities of the interplanetary magnetic field, the characteristic large-scale distribution of the background magnetic fields and the complex of solar activity.
碎石
发表于 2025-3-24 22:46:13
https://doi.org/10.1007/978-3-476-04221-7rray Magnetograph. The observations consist of time sequences of simultaneous velocity, magnetic field, and chromospheric network measurements. From these data it appears that the supergranular velocity cells have lifetimes in excess of 30 h. Magnetic field motions associated with supergranulation w
forestry
发表于 2025-3-25 00:49:49
https://doi.org/10.1007/978-3-476-03267-6 has been investigated using the polarity (toward or away from the Sun) of the interplanetary magnetic field as inferred from polar geomagnetic observations. The polarity of the interplanetary magnetic field has previously been shown to be closely related to the polarity (into or out of the Sun) of