Titlebook: Coronal Expansion and Solar Wind; A. J. Hundhausen Book 1972 Springer-Verlag Berlin · Heidelberg 1972 Korona (Astron.).Orbit.Scale.Sonnenw

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書目名稱Coronal Expansion and Solar Wind影響因子(影響力)




書目名稱Coronal Expansion and Solar Wind影響因子(影響力)學(xué)科排名




書目名稱Coronal Expansion and Solar Wind網(wǎng)絡(luò)公開度




書目名稱Coronal Expansion and Solar Wind網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Coronal Expansion and Solar Wind被引頻次




書目名稱Coronal Expansion and Solar Wind被引頻次學(xué)科排名




書目名稱Coronal Expansion and Solar Wind年度引用




書目名稱Coronal Expansion and Solar Wind年度引用學(xué)科排名




書目名稱Coronal Expansion and Solar Wind讀者反饋




書目名稱Coronal Expansion and Solar Wind讀者反饋學(xué)科排名

教育學(xué)

Nutrient

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Concluding Remarks,ures and processes, has led to the neglect of several interesting and important areas of solar wind research. Some mention of such areas, along with recent reviews and key works that will serve to guide the reader interested in their exploration, is in order. Introductory treatments of many of these topics have been given by Brandt [7.1].

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II–VI electroluminescent devices This era saw development of the basic concept of the solar wind as well as a model of its origin in the continuous expansion of the solar corona. Observations of a continuous supersonic flow of plasma and a magnetic field configuration fitting the expected pattern by the first spacecraft to probe i

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Bulk growth of widegap II–VI single crystalse chemical composition of the outer layers of the sun. Only two of the expected chemical constituents of the plasma, the ions .H. and .H. (where, in our notation, the left superscript denotes the atomic mass number and the right superscript denotes the ionic charge) have been routinely and extensive

舞蹈編排

Bulk growth of widegap II–VI single crystalsal solar wind. Mere inspection of solar wind data reveals large variations on a time scale of several days, comparable to the basic scale time of the overall coronal expansion (and thus indicative of phenomena in Class 2 of the classification scheme developed in Chapter II). Autocorrelation analysis