標(biāo)題: Titlebook: Solar and Interplanetary Dynamics; M. Dryer,E. Tandberg-Hanssen Book 1980 International Astronomical Union 1980 Variation.astrophysics.cos [打印本頁] 作者: Cataplexy 時(shí)間: 2025-3-21 17:55
書目名稱Solar and Interplanetary Dynamics影響因子(影響力)
書目名稱Solar and Interplanetary Dynamics影響因子(影響力)學(xué)科排名
書目名稱Solar and Interplanetary Dynamics網(wǎng)絡(luò)公開度
書目名稱Solar and Interplanetary Dynamics網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Solar and Interplanetary Dynamics被引頻次
書目名稱Solar and Interplanetary Dynamics被引頻次學(xué)科排名
書目名稱Solar and Interplanetary Dynamics年度引用
書目名稱Solar and Interplanetary Dynamics年度引用學(xué)科排名
書目名稱Solar and Interplanetary Dynamics讀者反饋
書目名稱Solar and Interplanetary Dynamics讀者反饋學(xué)科排名
作者: TERRA 時(shí)間: 2025-3-21 23:28
A Two-Level Solar Dynamo Based on Solar Activity, Convection, and Differential Rotationhere. It seems natural, therefore, to expect the reconnection aspect of conversion to be located there, where the least work needs to be performed. To transfer the generated flux there, we may add to conversion another spontaneous process: . of bipolar structure (Parker, 1955). To transfer the recon作者: ALIAS 時(shí)間: 2025-3-22 03:09
The Origin of Interplanetary Sectorsize the force-free condition, . × . = 0, and in fact make the more restrictive assumption that this region is current free. The magnetic field in this region can be derived from a solution to the Laplace equation.作者: 單獨(dú) 時(shí)間: 2025-3-22 05:23
Stellar Mass Flux and Coronal Heating by Shock Wavese and dissipation terms. The input parameters are the base pressure, the base temperature and the mechanical flux introduced at chromospheric level in form of shock waves. If these three parameters allow a solar wind expansion, the output results are the radial variations of the density, of the temp作者: infatuation 時(shí)間: 2025-3-22 12:48 作者: 文件夾 時(shí)間: 2025-3-22 16:58
Book 1980 be understood only by the coupling of solar and interplan- etary topics in an intimate observational and theoretical structure. This book, intended for active research scientists and advanced grad- uate students, is an important step in this direction. The background of solar and interplanetary dyn作者: 中和 時(shí)間: 2025-3-22 19:54 作者: Affable 時(shí)間: 2025-3-22 23:18 作者: 捐助 時(shí)間: 2025-3-23 03:40
K. V. Sheridan,G. A. Dulkl ein besonders gesch?ftiges Jahr. Wie Richard Bellman es ausdrückte: ?Man wu?te nie, wo Erd?s sich gerade aufhielt, nicht einmal das Land kannte man. Aber man konnte sicher sein, da? er im Laufe eines ganzen Jahres überall erschien. Er kam einem ergodischen Teilchen [eines, das schlie?lich alle phy作者: 禁止 時(shí)間: 2025-3-23 08:19 作者: Infuriate 時(shí)間: 2025-3-23 12:29
V. Letfus,L. Kul?ár,J. SykoraThe Wall Street Journal .Mein Ich, die anderen und wir.ist dann besonders aufschlussreich, wenn Little über die polarisierenden Kategorien hinausgeht und zum Beispiel die Auswirkungen unserer Pers?nlichkeiten auf das erkundet, was er unsere ?pers?nlichen Projekte“ nennt.. .New York Times Book Review作者: Favorable 時(shí)間: 2025-3-23 17:47
S. W. Kahlerrma?nahmen dr?ngen und verlieren Ihre intuitive Sicherheit im Umgang mit dem Kind. Das Buch von Monika Aly m?chte Sie mit sachlicher Information und praktischem Rat darin unterstützen, die für Ihr Kind richtigen Entscheidungen zu treffen.978-3-540-42319-5978-3-642-56264-8作者: GRIN 時(shí)間: 2025-3-23 20:10 作者: Amnesty 時(shí)間: 2025-3-23 23:39
J. N. Tandonrma?nahmen dr?ngen und verlieren Ihre intuitive Sicherheit im Umgang mit dem Kind. Das Buch von Monika Aly m?chte Sie mit sachlicher Information und praktischem Rat darin unterstützen, die für Ihr Kind richtigen Entscheidungen zu treffen.978-3-540-42319-5978-3-642-56264-8作者: Lumbar-Spine 時(shí)間: 2025-3-24 05:23 作者: SEED 時(shí)間: 2025-3-24 06:42 作者: Stable-Angina 時(shí)間: 2025-3-24 12:10
C. D’Uston,J. M. Bosqued. — An der Grenzstation Kufstein wurde ich in der Nacht von einem deutschen Beamten aus dem Waggon geholt. Ich mu?te mit meinem Gep?ck ins Stationsgeb?ude, wo man mir alle Taschen umkehrte und mich bis aufs Hemd untersuchte. Die paar hundert Lire, die ich über die erlaubte Summe hinaus mit mir hatte作者: 流逝 時(shí)間: 2025-3-24 18:48 作者: 使?jié)M足 時(shí)間: 2025-3-24 23:05
Evolution of Coronal and Interplanetary Magnetic Fieldsthe sun and the structure of the interplanetary field. We will point out the latest techniques and studies of the global solar magnetic field and its relation to the interplanetary field.. The potential to overcome most of the limitations of present methods of analysis exists in techniques of modell作者: Obvious 時(shí)間: 2025-3-25 01:08
Search for Giant Cells in the Solar Convection Zoneetogram is taken, the position of the Doppler line shift compensator is also recorded, thus giving a full disk map of the longitudinal velocity. This entire dataset is currently being rereduced on a uniform basis (Howard et al., 1980), and daily arrays of residual velocities are being formed by remo作者: limber 時(shí)間: 2025-3-25 06:04
Dynamics of Large-Scale Magnetic Field Evolution During Solar Cycle 204. The results include: a unique magnetic pattern coinciding with major coronal holes; variations in the rate of solar rotation through the solar cycle; discovery of convergence and divergence among long-lived magnetic patterns; periodic discontinuities in the organization of large-scale magnetic fi作者: intrude 時(shí)間: 2025-3-25 07:29
A Two-Level Solar Dynamo Based on Solar Activity, Convection, and Differential Rotation both located in the high β regime convection zone. . requires that regime, since its function demands it be driven by mechanical forces. But the function and therefore the operating requirements of . are entirely different, and there seems to be no à . reason, other than historical tradition couple作者: disrupt 時(shí)間: 2025-3-25 13:44 作者: 搖擺 時(shí)間: 2025-3-25 18:41
Radio Observations of Coronal Holesreas of low brightness, either on the disk or at the limb. At 80 MHz holes on the limb always appear less bright than their surroundings but on the disk they frequently appear brighter..The simplest interpretation is that the coronal temperature in holes near the 80 MHz critical density (8 × 10. cm.作者: 哪有黃油 時(shí)間: 2025-3-26 00:04
A Model for the North Coronal Hole Observed at the 1973 Eclipse, Between 1.3 and 3.2 R⊙y-compensated filter. These pictures provide a very good opportunity for studying the large coronal hole at the north polar cap; this hole has been extensively studied during the Skylab period. On the plates of Koutchmy, we could record reliable intensities between 1.3 and 3.2 R . The absolute calib作者: 橫截,橫斷 時(shí)間: 2025-3-26 00:52
Solar Observations with a New Earth-Orbiting Coronagraphpproximately 1.25 arc min and a repetition rate of 10 minutes during the one-hour sunlit portion of each 97-minute satellite orbital period. These are the first satellite observations of the outer corona near the peak of a sunspot cycle when coronal transients and high-latitude streamers are common.作者: Afflict 時(shí)間: 2025-3-26 05:39 作者: MAOIS 時(shí)間: 2025-3-26 11:38
The Origin of Interplanetary Sectorsoronal magnetic field from the observed photospheric magnetic field shed light on the origin of sectors. Figure 1 from Schatten’s (1971) “Current Sheet Model” is a schematic representation of these similar models. There are three distinct regions in these models where different physical phenomena oc作者: 勤勞 時(shí)間: 2025-3-26 14:49
Coronal Structure and Solar Windned through the focussing of solar-ion streams taking account of the local and general solar magnetic fields. This explains the association of coronal holes with weak, diverging open magnetic field lines and envisages the transfer of hydromagnetic wave energy from nearby active centers to account fo作者: legitimate 時(shí)間: 2025-3-26 19:26 作者: Sarcoma 時(shí)間: 2025-3-26 21:03
Interplanetary Response to Solar Long Time-Scale Phenomenana such as the coronal magnetic structure and its evolution. Observational evidence that solar wind flow in the outer corona comes from the unipolar diverging magnetic regions of the photosphere is discussed along with relations to coronal holes. High-speed solar wind streams observed within the bou作者: 得意人 時(shí)間: 2025-3-27 02:50 作者: MOAN 時(shí)間: 2025-3-27 09:20
Reflexion and Transmission of Alfven Waves in an Atmospherehree MHD modes. Here, we will consider linear Alfvén waves only. The problem is set as follows. An energy flux being given at the bottom (z=0) of the atmosphere, we ask for how much of it is recorded at an altitude z.作者: euphoria 時(shí)間: 2025-3-27 11:35 作者: Alveoli 時(shí)間: 2025-3-27 14:37 作者: 障礙物 時(shí)間: 2025-3-27 21:45
Search for Giant Cells in the Solar Convection Zoneentire dataset is currently being rereduced on a uniform basis (Howard et al., 1980), and daily arrays of residual velocities are being formed by removing large scale patterns, e.g., Earth’s motions, solar rotation, limbshift. Data from the years 1972 through 1978 are used here.作者: modish 時(shí)間: 2025-3-28 01:15 作者: slow-wave-sleep 時(shí)間: 2025-3-28 02:43
Radio Observations of Coronal Holessk they frequently appear brighter..The simplest interpretation is that the coronal temperature in holes near the 80 MHz critical density (8 × 10. cm.) is higher than in normal quiet regions, but that the density at this level is lower.作者: Oafishness 時(shí)間: 2025-3-28 08:56
Coronal Structure and Solar Wind holes with weak, diverging open magnetic field lines and envisages the transfer of hydromagnetic wave energy from nearby active centers to account for the enhanced outflow of solar wind associated with coronal holes.作者: 步兵 時(shí)間: 2025-3-28 12:55 作者: 耕種 時(shí)間: 2025-3-28 17:05 作者: RALES 時(shí)間: 2025-3-28 20:08
Evolution of Coronal and Interplanetary Magnetic Fieldsven heliospheric point and its magnetically-connected photospheric point, as well as the physical basis for the connection. We thus find ourselves at a plateau, looking back over a quarter century of empirical synthesis while anticipating a new era of detailed physical investigation on a global scale.作者: 不愛防注射 時(shí)間: 2025-3-29 00:48
X-Ray Structures Associated with Disappearing Hα Filaments in Active Regionsding loops associated with an active region filament which disappeared. Rust and Webb (1977) found a good statistical correlation in time and position between large scale (length > 60, 000 km) active region X-ray enhancements and Hα filament activity, in particular, events of an eruptive nature.作者: outskirts 時(shí)間: 2025-3-29 04:08
Book 1980e two often-divergent groups. It was clear that the latter group was dependent essentially on the sun for its raison d‘etre. On the other hand it was also clear that the former group could benefit in its search for insight vis-a-vis solar activity by looking beyond the shell of the inner corona. Nee作者: 無表情 時(shí)間: 2025-3-29 09:48
A Model for the North Coronal Hole Observed at the 1973 Eclipse, Between 1.3 and 3.2 R⊙ration was made using the stars observed in the field at the same time. This method allows a direct comparison of well-exposed objects on a same plate and must therefore be highly reliable (see Koutchmy et al., 1978). It is well-known that the absolute calibration of eclipse plates is a difficult problem.作者: 無脊椎 時(shí)間: 2025-3-29 14:52 作者: Mri485 時(shí)間: 2025-3-29 19:26 作者: 極大的痛苦 時(shí)間: 2025-3-29 23:25
978-90-277-1163-2International Astronomical Union 1980作者: 土坯 時(shí)間: 2025-3-30 03:22 作者: Cacophonous 時(shí)間: 2025-3-30 04:10 作者: cancellous-bone 時(shí)間: 2025-3-30 10:55
https://doi.org/10.1007/978-94-009-9100-2Variation; astrophysics; cosmic ray; dynamics; galaxies; heliosphere; planet; solar activity; solar system; s作者: CAND 時(shí)間: 2025-3-30 15:09 作者: 兩種語言 時(shí)間: 2025-3-30 16:46
The Coronal Responses to the Large-Scale and Long-Term Phenomena of the Lower Layers of the SunBased on the assumption, generally accepted over the past decade, that all the forms of solar and interplanetary activity are responses to the magnetic fields generated initially in the subphotosphere, some characteristics of the large-scale and long-term behaviour of the solar corona during the last three solar cycles are presented.作者: 膝蓋 時(shí)間: 2025-3-30 23:04 作者: Keratin 時(shí)間: 2025-3-31 04:38
Solar Observations with a New Earth-Orbiting Coronagraphpproximately 1.25 arc min and a repetition rate of 10 minutes during the one-hour sunlit portion of each 97-minute satellite orbital period. These are the first satellite observations of the outer corona near the peak of a sunspot cycle when coronal transients and high-latitude streamers are common.作者: 宮殿般 時(shí)間: 2025-3-31 06:06 作者: 滑動(dòng) 時(shí)間: 2025-3-31 13:02
V. Gaizauskas,K. F. Tappinggen, Flugzeugen und Koffern, die mit Aufklebern aus exotischen L?ndern beklebt waren. 1960 zum Beispiel reiste Erd?s in Windeseile von Budapest nach Moskau, dann nach Leningrad, zurück nach Moskau und schlie?lich nach Peking via Irkutsk und Ulan Bator. Nach drei Wochen in Peking, in denen er sich mi作者: orient 時(shí)間: 2025-3-31 17:11
K. V. Sheridan,G. A. Dulkgen, Flugzeugen und Koffern, die mit Aufklebern aus exotischen L?ndern beklebt waren. 1960 zum Beispiel reiste Erd?s in Windeseile von Budapest nach Moskau, dann nach Leningrad, zurück nach Moskau und schlie?lich nach Peking via Irkutsk und Ulan Bator. Nach drei Wochen in Peking, in denen er sich mi作者: maroon 時(shí)間: 2025-3-31 18:21 作者: 群居動(dòng)物 時(shí)間: 2025-4-1 01:43 作者: 火海 時(shí)間: 2025-4-1 02:01
S. W. Kahlers illustriert - in der Neuauflage durchgehend farbig!.IncludHaben Sie das Gefühl, dass bei Ihrem Baby "etwas" nicht stimmt? Vielleicht hat es einfach die Folgen seiner zu frühen Geburt noch nicht verkraftet; vielleicht beobachten Sie aber Anzeichen, die auf eine schwer wiegende Entwicklungsst?rung h作者: archaeology 時(shí)間: 2025-4-1 07:01 作者: 強(qiáng)制令 時(shí)間: 2025-4-1 11:35
J. N. Tandons illustriert - in der Neuauflage durchgehend farbig!.IncludHaben Sie das Gefühl, dass bei Ihrem Baby "etwas" nicht stimmt? Vielleicht hat es einfach die Folgen seiner zu frühen Geburt noch nicht verkraftet; vielleicht beobachten Sie aber Anzeichen, die auf eine schwer wiegende Entwicklungsst?rung h作者: overrule 時(shí)間: 2025-4-1 15:01
H. S. AhluwaliaFahrt nach dem Osten und damit zugleich die erste Gelegenheit, einen Eindruck zu bekommen von der Vormacht des englischen Volkes. Wir waren bisher immer nur nach den südlichen L?ndern Europas gereist, nach Frankreich, Italien und Dalmatien, und hatten wenig Ahnung von der kolonisierenden Kraft und d作者: 嬉耍 時(shí)間: 2025-4-1 22:30 作者: 腐爛 時(shí)間: 2025-4-1 23:35 作者: 賄賂 時(shí)間: 2025-4-2 04:16 作者: depreciate 時(shí)間: 2025-4-2 07:26 作者: airborne 時(shí)間: 2025-4-2 14:28 作者: linguistics 時(shí)間: 2025-4-2 17:07
,Selbstorganisationsprozesse in Unternehmen — Zu den Perspektiven demokratischen Wirtschaftens,undert die verschiedensten politischen Weltanschauungen und Theorieangebote auf sich gezogen hat. Diese miteinander zu verknüpfen ist mindestens im Rahmen eines Vortrags ein v?llig unm?gliches Unterfangen. Angesichts der Theoriegeschichte einiger hier Anwesender, meine eigene Person eingeschlossen, 作者: 使顯得不重要 時(shí)間: 2025-4-2 22:15 作者: GRAZE 時(shí)間: 2025-4-3 02:24
Jean-Daniel Bancaltreitgegenstandes sowie eine verbindliche richterliche Entscheidung in angemessener Zeit. gew?hrleistet.. Nichts anderes gilt für das Verh?ltnis zwischen Individuum und Staat.. Die nicht zuletzt aus historischen Gründen (vgl. dazu oben § 2 Rdnr. 2) problematische Doppelrolle, in der sich der Staat b
