標(biāo)題: Titlebook: Coronal Expansion and Solar Wind; A. J. Hundhausen Book 1972 Springer-Verlag Berlin · Heidelberg 1972 Korona (Astron.).Orbit.Scale.Sonnenw [打印本頁] 作者: GLAZE 時間: 2025-3-21 16:11
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
作者: 教育學(xué) 時間: 2025-3-21 20:40 作者: Nutrient 時間: 2025-3-22 02:05 作者: Cuisine 時間: 2025-3-22 08:29 作者: LITHE 時間: 2025-3-22 12:26
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].作者: 吞噬 時間: 2025-3-22 14:47 作者: 吞噬 時間: 2025-3-22 18:32
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作者: 偉大 時間: 2025-3-22 22:20 作者: 會犯錯誤 時間: 2025-3-23 02:03
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作者: 舞蹈編排 時間: 2025-3-23 07:22
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作者: 迅速成長 時間: 2025-3-23 12:38 作者: Kindle 時間: 2025-3-23 17:06
Bulk growth of widegap II–VI single crystalsures 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作者: 思想靈活 時間: 2025-3-23 20:35
Physics and Chemistry in Spacehttp://image.papertrans.cn/c/image/238290.jpg作者: 要求比…更好 時間: 2025-3-24 01:29 作者: heartburn 時間: 2025-3-24 05:10
The Identification and Classification of Some Important Solar Wind Phenomena, 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作者: LUCY 時間: 2025-3-24 06:59
The Dynamics of a Structureless Coronal Expansion,y 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作者: AGOG 時間: 2025-3-24 12:14 作者: 誘惑 時間: 2025-3-24 15:34
High-Speed Plasma Streams and Magnetic Sectors,al 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作者: 不真 時間: 2025-3-24 21:24
Flare-Produced Interplanetary Shock Waves,l ejected by the flare. Consider a volume of this material, presumably plasma from the chromosphere or low corona, moving rapidly outward into a slower ambient solar wind (such as already shown in Fig. 5.9). Fig. 6.1 shows a hypothetical cross section (in the solar equatorial plane) of the resulting作者: Legion 時間: 2025-3-25 00:03 作者: 星星 時間: 2025-3-25 07:18 作者: 滑動 時間: 2025-3-25 10:11
II–VI electroluminescent deviceservations of a continuous supersonic flow of plasma and a magnetic field configuration fitting the expected pattern by the first spacecraft to probe interplanetary space demonstrated the fundamental validity of this concept and theory.作者: formula 時間: 2025-3-25 15:34
Bulk growth of widegap II–VI single crystalsr ambient solar wind (such as already shown in Fig. 5.9). Fig. 6.1 shows a hypothetical cross section (in the solar equatorial plane) of the resulting solar wind disturbance at a time when it has traveled well out into interplanetary space. 作者: infatuation 時間: 2025-3-25 19:17
Book 1972ons 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 the interpl作者: Ordeal 時間: 2025-3-25 21:12 作者: 集聚成團(tuán) 時間: 2025-3-26 01:15 作者: nascent 時間: 2025-3-26 04:19 作者: 食料 時間: 2025-3-26 12:18 作者: glucagon 時間: 2025-3-26 14:15 作者: monogamy 時間: 2025-3-26 17:12
Chemical Composition of the Expanding Coronal and Interplanetary Plasma, the polarization electric field of the coronal plasma, as already described in I.6. Ions other than .H. and .H. can be observed by present day plasma detectors only under favorable (and rare) circumstances. These infrequent observations have led to some knowledge of the interplanetary abundance of 作者: Flatter 時間: 2025-3-26 21:51 作者: Ceremony 時間: 2025-3-27 03:18 作者: Ingredient 時間: 2025-3-27 08:31
0079-1938 ing in the coronal and interplanetary plasma and as the natural manifestations of solar properties and structures. This approach implies an emphasis upon the "l978-3-642-65416-9978-3-642-65414-5Series ISSN 0079-1938 作者: Asperity 時間: 2025-3-27 10:19 作者: 雪白 時間: 2025-3-27 13:40 作者: 呼吸 時間: 2025-3-27 19:34
Bulk growth of widegap II–VI single crystalsnetary space would then result from rotation of this spatial structure past the observer. The polarity of the interplanetary magnetic field has also been found to be organized into unipolar regions with a similar scale size (or time), that are related to the high-speed streams. We will now review th作者: BRAWL 時間: 2025-3-28 01:54 作者: Hippocampus 時間: 2025-3-28 05:59 作者: 碌碌之人 時間: 2025-3-28 09:24 作者: 赤字 時間: 2025-3-28 10:32
Norbert Schappacherin zwei Bundesministerien sowie in leitender Funktion bei einem gro?en Energieunternehmen t?tig und ist Lehrbeauftragter in verschiedenen Masterstudieng?ngen an der RWTH Aachen..Aus dem Inhalt.-? ? ? ??.? Grundlagen der Energiewirtschaft.-????????? Struktur einzelner Energie-Teilm?r978-3-658-23024-1作者: 并排上下 時間: 2025-3-28 15:44
