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Large-Scale Magnetic Fields and Activity Patterns on the Sun at least four cycles. This means that the organization of activity and fields in streams or active longitudes does not change during several tens of years and proceeds in the same way following the same rules of development, (c) . may also play a role in the formation of large-scale patterns..The dbronchiole 发表于 2025-3-22 03:26:17
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Time Variations in Solar Activityer corresponded to recognizable episodes in specific solar activity and to maxima in plots of Major Flare and Active Region Indices..Study of the declining branches of solar cycles 12 through 19 suggests that there will be 5 to 6 Primary Fluctuations of activity on the declining branch of cycle 20 ireflection 发表于 2025-3-22 15:06:53
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Scattering and Scintillations of Discrete Radio Sources as a Measure of the Interplanetary Plasma Ir component of the velocity of motion of the diffraction pattern Y. These quantities are functions of the time and location of the ray relative to the Sun (sometimes expressed as the angular distance or elongation ε of the source from the Sun, sometimes as the linear distance .); and all but the lastLacunar-Stroke 发表于 2025-3-23 01:17:45
Galactic Cosmic Ray Modulation by the Interplanetary Medium (Including the Problem of the Outer Bounproperties of the solar wind at the boundary with the interstellar medium are estimated. The turbulent transition zone of the subsonic solar wind and its possible effect on the galactic cosmic rays are studied.知识分子 发表于 2025-3-23 02:18:50
A. Bruzeklls..Cutting-edge and thorough, .Melatonin: Methods and Protocols. is a valuable resource for any researcher interested in investigating melatonin, from its production to its mec978-1-0716-2595-8978-1-0716-2593-4Series ISSN 1064-3745 Series E-ISSN 1940-6029BURSA 发表于 2025-3-23 08:25:59
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