贪求
发表于 2025-3-21 16:18:42
书目名称Cosmical Magnetism影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0238904<br><br> <br><br>书目名称Cosmical Magnetism读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0238904<br><br> <br><br>
FLAGR
发表于 2025-3-21 23:00:22
Introduction: Making the Medicinal Poisoner,ing magnetic features that are usually observed to be present in the photosphere below bright points. The model has three phases: a preinteraction phase in which two opposite polarity photospheric magnetic fragments are unconnected magnetically; an interaction phase when the fragments reconnect in t
抵消
发表于 2025-3-22 04:11:16
Learning at Home and on the Shop Floor a high temperature of 10.K, and occasionally producing spectacular solar flares. The energy flux needed to balance the losses by radiation or by the solar wind of non-flaring coronal gas ranges between several 10. ergs cm. . . in quiet regions to 10. ergs cm. . . in active regions. Coronal holes do
EXULT
发表于 2025-3-22 07:22:52
From Globalisation to Industrialisationinfluence the theory of the evolution of Cataclysmic Variables, ii) the instability of the toroidal field component in winds and jets from accretion disks, iii) the importance of poloidal vs toroidal collimation of jets, and iv) what determines the distribution of field strength in the disk from whi
字谜游戏
发表于 2025-3-22 09:12:39
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扫兴
发表于 2025-3-22 16:49:06
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扫兴
发表于 2025-3-22 18:36:27
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ungainly
发表于 2025-3-22 22:15:59
Introduction: The Written Constitution,equences include the formation of weak dipole moment millisecond pulsars by the accretion induced spin-up of strong field neutron stars, the absence of observable spin modulation of the thermal X-ray emission from the surfaces of neutron stars in accreting low mass X-ray binaries (LMXB’s), pulsar pe
instate
发表于 2025-3-23 05:17:42
Introduction: The Written Constitution,fects need to be taken into account in the equation of motion. When this happens, a quasi-classical description is required, with deterministic trajectories becoming stochastic, because quantum corrections must be considered. In this paper the associated physical processes are discussed, simultaneou
Omniscient
发表于 2025-3-23 09:27:37
Introduction: The Written Constitution,ments by cosmic-ray spallation on interstellar CNO nuclei. Several solutions have been proposed, including confinement of cosmic rays by a strong magnetic field in the early Galaxy, but none of them is very satisfactory. In this paper I suggest a chemically inhomogeneous model for the halo which may