银河
发表于 2025-3-21 17:56:42
书目名称Informatik — Wirtschaft — Gesellschaft影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0464967<br><br> <br><br>书目名称Informatik — Wirtschaft — Gesellschaft读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0464967<br><br> <br><br>
会犯错误
发表于 2025-3-21 23:27:10
passively, in virtually all coronal disturbances. The purpose of this paper is to put into perspective the various roles magnetic fields can play in both exciting and guiding these observed transient phenomena. A discussion of our present theoretical concepts relevant to this subject can be convenie
法官
发表于 2025-3-22 03:50:20
B. Shriversisted of A. Boischot, A. Bruzek, J. T. Jefferies, G. Newkirk, T. Takakura, and V. V. Zhelez nyakov. We are indebted to the Local Organizing Commettee, chaired by S. F. Smerd and including R. G. Giovanelli, R. E. Loughhead, N. G. Seddon, K. V. Sheridan, and J. P. Wild, for advice in preparing this
Cognizance
发表于 2025-3-22 07:47:36
W. Wahlster observations con firmed the basic validity of a theoretical model, first proposed by E. N. Parker, predicting a continuous, rapid expansion of the solar corona. The subsequent decade has seen a tremendous growth in both the breadth and sophistication of solar wind observations; the properties of t
进步
发表于 2025-3-22 10:52:41
Klaus Lenky discussion of the physics of the interplanetary plasma. We have already seen that the models of Parker, based on the assumption of steady, spherically-symmetric fluid motion, correctly predicted the basic characteristics of the solar wind. The adoption of this same simplifying assumption in the fo
intellect
发表于 2025-3-22 16:03:18
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Insensate
发表于 2025-3-22 19:56:51
Britta Schinzelobservations, which contain a last part of the maximum phase of the solar cycle 22, it was possible to obtain almost every aspect of solar activity at 17 GHz. They include two X-class flares, tens of M-class flares, hundreds of flares from the very initial phase through the late decay phase, or from
Accede
发表于 2025-3-23 00:01:32
Frieder Nakeobservations, which contain a last part of the maximum phase of the solar cycle 22, it was possible to obtain almost every aspect of solar activity at 17 GHz. They include two X-class flares, tens of M-class flares, hundreds of flares from the very initial phase through the late decay phase, or from
正式通知
发表于 2025-3-23 03:28:50
EREO/COR1 data obtained during a deep minimum of solar activity in February 2008 (Carrington Rotation CR 2066) to retrieve and analyze the three-dimensional (3D) coronal electron density in the range of heights from 1.5 to 4 R. using a tomography method. With this, we qualitatively deduced structure
leniency
发表于 2025-3-23 06:55:58
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