Enlightening
发表于 2025-3-21 19:22:54
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谁在削木头
发表于 2025-3-21 22:00:33
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debunk
发表于 2025-3-22 03:38:59
Uwe ChristiansLehnert, took the first steps towards its realization. - ESRIN readily adopted this idea, and preliminary contacts with a number of other groups showed that there was a good deal of interest in bringing to gether people working in different areas of the field of cosmic plasma physics. It was clearl
Aqueous-Humor
发表于 2025-3-22 07:42:25
Wilhelm Schmeisserat, as an aid to detailed understanding, please return with pencil and paper to work out the missing steps (if any) in the formal mathematics. On the basis of such an approach the student interested in modern astro physics, its current practice, will find the answers to two key questions: (1) what
摇曳的微光
发表于 2025-3-22 10:02:36
Wilhelm Schmeisser,Marko Gallerom complete samples of quasars. We first concentrate on optical survey of quasars. For quasars of medium luminosity, the co-moving space density rises very steeply with redshift. Quasars of lower luminosity exhibit a slower increase of density with redshift, resulting in luminosity-dependent evoluti
NADIR
发表于 2025-3-22 13:30:37
Gerfried Hannemann,Wilhelm Schmeissere existence of some form of “new physics” beyond the standard model. The evidence for the existence of new physics is based on the observation of three effects: (i) a measured μ/e ratio smaller that the expectation, (ii) the detection of a strong up/down asymmetry for μ-like events, and (iii) the di
烧瓶
发表于 2025-3-22 18:03:53
Wilhelm Schmeissery cosmic rays. Simpson (1948) discovered that the latitude variation of the secondary hadronic component was considerably larger than the muon component suggesting the response of a neutron monitor is more sensitive to lower energies in the primary spectrum. The different methods of determining the
Defiance
发表于 2025-3-22 23:35:58
Daniel M. Evanstudy of cosmic ray spectra, time variations, abundances, gradients, and anisotropy provides a wealth of data on physical conditions in the regions of cosmic ray generation as well as in the media through which cosmic rays propagate. Astrophysical aspects of cosmic ray physics have been considered in
Physiatrist
发表于 2025-3-23 02:22:32
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congenial
发表于 2025-3-23 05:41:50
Manfred Kühnberger,Thomas Grubernd negative magnetic polarities are observed, and by the unipolar regions above and below the sector zone. Distinct corotating streams and interactions regions are found primarily in the sector zone during the declining phase of the solar cycle. Within a few AU, the streams and interaction regions a