標題: Titlebook: Activity in Red-Dwarf Stars; Proceedings of the 7 Patrick B. Byrne,Marcello Rodonò Conference proceedings 1983 Springer Science+Business Me [打印本頁] 作者: 譴責 時間: 2025-3-21 16:29
書目名稱Activity in Red-Dwarf Stars影響因子(影響力)
書目名稱Activity in Red-Dwarf Stars影響因子(影響力)學科排名
書目名稱Activity in Red-Dwarf Stars網(wǎng)絡公開度
書目名稱Activity in Red-Dwarf Stars網(wǎng)絡公開度學科排名
書目名稱Activity in Red-Dwarf Stars被引頻次
書目名稱Activity in Red-Dwarf Stars被引頻次學科排名
書目名稱Activity in Red-Dwarf Stars年度引用
書目名稱Activity in Red-Dwarf Stars年度引用學科排名
書目名稱Activity in Red-Dwarf Stars讀者反饋
書目名稱Activity in Red-Dwarf Stars讀者反饋學科排名
作者: 動物 時間: 2025-3-21 23:34
Global and Photospheric Physical Parameters of Active Dwarf Starstungsweise) der Disziplin sowie der Abgrenzung gegenüber anderen Wissenschaften kann man sinnvollerweise erst dann sprechen, wenn hinsichtlich der Frage ?reine oder angewandte Wissenschaft” Einigkeit besteht., was nicht selten übersehen wird.. Bevor wir indessen auf den Unterschied zwischen ?reinen“作者: Minuet 時間: 2025-3-22 01:36 作者: Euthyroid 時間: 2025-3-22 07:06
The Structure and Energy Balance in Main Sequence Starsbe severely trimmed and skimmed to fit “neatly” into the selected concepts. As local researchers provide evidence that what was found in the West is also to be found in an Asian context, the universalizing claim of Western concepts is (re-)affirmed. Both processes are unhappy ones, even if there wer作者: Ostrich 時間: 2025-3-22 12:32 作者: 游行 時間: 2025-3-22 13:42
Late-Type Ca II Emission-Line Stars in the Southern Hemisphere invited speakers. The aim was to get the participants aware of the current state of the art and to highlight the main outstanding issues. The second day consisted of the Workshop participants splitting into three groups and discussing specific issues in depth. Plenary sessions helped to keep the individual g978-3-642-70921-0978-3-642-70919-7作者: 敘述 時間: 2025-3-22 20:25 作者: 使饑餓 時間: 2025-3-22 23:12
Some Properties of Stellar Transition Regions, status of the big cat remains precarious. Rigorous monitoring of surviving wild tiger populations continues to be essential for both understanding and recovering wild tigers. However, many tiger monitoring programs lack the necessary rigor to generate the reliable results. While the deployment of 作者: BOON 時間: 2025-3-23 04:02
Quiescent Coronae of Active Chromosphere Starsne metabolism, uric acid. Thus it has been proposed that a potent inhibitor of PNP might serve as a biochemical modifier in chemotherapy with purine nucleoside analogs, as a selective immunosuppressive agent, and perhaps in the treatment of secondary gout (Parks .., 1981; Stoeckler .., 1980a, 1982; 作者: Cantankerous 時間: 2025-3-23 07:18
Einstein and IUE Observations of Nearby Red Dwarfsfor a proper literature appraisal.. Addressing that gap, this book discusses more practical aspects of clinical research and biostatistics in oncology, instead of relying only on mathematical formulas and theoretical considerations. Methods and Biostatistics in Oncology will help readers develop the作者: 天然熱噴泉 時間: 2025-3-23 10:03 作者: PATHY 時間: 2025-3-23 17:05
e for many years, and the resolution advantage of electron beam and X-ray methods will not be needed except in research and development. An exception to this is when fast turnaround is an asset such as in mask making and gate-array personalization. Here scanning electron beams are very valuable. The作者: 辯論 時間: 2025-3-23 20:54
Optical Photometry of Flares and Flare Statisticstially influenced by the selection of rating scales and decision rules. Therefore, the rating scales and decision rules should be carefully defined and discussed among the research teams. In our case, experts have participated from five European countries.作者: Neuropeptides 時間: 2025-3-23 23:20 作者: 符合國情 時間: 2025-3-24 06:00
Speicherprogrammierbare Steuerungen.Arguments are presented in support of the hypothesis that M-dwarf coronae are magnetically dominated, as is the Solar corona. We then examine the usefulness of loop model atmosphere calculations in elucidating the coronal heating mechanism and the ways in which observations may be used to test comp作者: 伸展 時間: 2025-3-24 08:52
0067-0057 as posters. It is gratifying that in the short time since the meeting a good deal of correspondence has been received from participants remarking on the succes978-94-009-7159-2978-94-009-7157-8Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 小樣他閑聊 時間: 2025-3-24 11:15
Front Matter (such as elevators, thermo-technical plants, etc.). The author also discusses the usage of ad hoc designed software analysis tools based on neural networks and reliability indicators.Methodologies and Techniqu978-1-4471-5723-6978-0-85729-103-5作者: 小溪 時間: 2025-3-24 18:19 作者: fatty-acids 時間: 2025-3-24 22:58 作者: Fluctuate 時間: 2025-3-25 02:23 作者: medieval 時間: 2025-3-25 05:30
Spots, Spot-Cycles and Magnetic Fields of Late-Type Dwarfs978-3-030-27045-2作者: CRUMB 時間: 2025-3-25 09:24 作者: RUPT 時間: 2025-3-25 12:34 作者: POWER 時間: 2025-3-25 16:07 作者: DEBT 時間: 2025-3-25 21:15
Automatisierung von FührungsentscheidungenThe results of a photometric and spectroscopic study of twenty-three late-type southern stars with strong Ca II H and K emission are presented.作者: 偏狂癥 時間: 2025-3-26 01:57
Erzeugung von Terminierungshypothesen,Among the strongest lines from stellar transition regions are the resonance lines of N V (1240?), Si IV (1394, 1403?), and C IV (1549?), which are all observable by the IUE.作者: transplantation 時間: 2025-3-26 08:06 作者: 吹牛大王 時間: 2025-3-26 11:00 作者: 發(fā)炎 時間: 2025-3-26 15:49 作者: 苦澀 時間: 2025-3-26 19:07 作者: 表主動 時間: 2025-3-27 00:53
https://doi.org/10.1007/978-3-642-61435-4 solar-type stars) and similarly high fluxes of chromospheric and transition region line fluxes compared to the Sun (Stern et al.1981, Zolcinski et al. 1981, 1982). A giant x-ray flare from a spectroscopic binary system in the Hyades has also been reported (Stern, Antiochos and Underwood 1982).作者: Flat-Feet 時間: 2025-3-27 03:07
Stefan Roth,Anna Priester,Christopher Pützernational Astronomical Union on “Activity in Red-Dwarf Stars”. First of all let me thank all of you for accepting our invitation to attend the Opening Ceremony. Such an impressive gathering of so many distinguished astrophysicists from all over the world is in itself a reward for all of us in the S作者: insular 時間: 2025-3-27 08:13
Stefan Roth,Anna Priester,Christopher Pützdetermined for quiescent conditions. The interrelations between these quantities are compared to the results of theoretical investigations for low mass stars. The evolutionary state of flare stars is discussed. Observational results from spectroscopic and photometric methods to determine the rotatio作者: mechanical 時間: 2025-3-27 12:53
https://doi.org/10.1007/978-3-8348-8251-6olor indices B-V, V-R, etc. for each spectral type. Such a table relates the observed colors of unreddened stars to their temperature classes and enables one to draw a reference line representing the main sequence on any color-color diagram.作者: Commemorate 時間: 2025-3-27 16:43
Automatisierung von Führungsentscheidungen Cen A, α Cen B and ε Eri. The EUV observations are combined with X-ray fluxes to predict the coronal temperatures, the electron pressures and energy lost or transferred by radiation and thermal conduction作者: SNEER 時間: 2025-3-27 19:58 作者: synovium 時間: 2025-3-27 21:55 作者: Repetitions 時間: 2025-3-28 03:34
Speicherprogrammierbare Steuerungen. We now have observed a sufficient number of the nearby M-dwarfs to determine an X-ray luminosity function and we have explored the activity and variability of these stars to the extent of observing, for the first time, X-ray flares with simultaneous ground-based optical and IUE ultraviolet coverag作者: 混合 時間: 2025-3-28 08:30
https://doi.org/10.1007/978-3-642-61435-4. The coronal X-ray, chromospheric ultraviolet, and auxiliary optical properties of sets of these stars are tabulated or illustrated in several ways. Factors of stellar duplicity are shown to be quite prevalent in presenting the observations. The most luminous X-ray dwarfs below the Sun are strongly作者: fabricate 時間: 2025-3-28 12:44
Speicherprogrammierbare Steuerungenre characterized by the presence of chromospheric emission lines like H. and CaII H and K which are present even during the quiescent state. The presence of transition regions and coronae have been inferred from the detection of UV emission lines like NV, CIV, SilV etc. with IUE and X-ray observatio作者: elastic 時間: 2025-3-28 17:11 作者: 時間等 時間: 2025-3-28 20:54 作者: analogous 時間: 2025-3-29 02:07
ph-Wert, Redoxspannung, Leitf?higkeite past and one might mention in particular Kunkel (1975), Gershberg (1978) and Gurzadyan (1980). In general these have been more broadly based than the present review incorporating other aspects of flare stars e.g. BY Dra variability, spectroscopic observations, etc. Since these other aspects of fla作者: Phonophobia 時間: 2025-3-29 03:46 作者: Traumatic-Grief 時間: 2025-3-29 08:17 作者: 不合 時間: 2025-3-29 14:48 作者: 集合 時間: 2025-3-29 18:04 作者: inundate 時間: 2025-3-29 19:46
Global and Photospheric Physical Parameters of Active Dwarf Starsegenübergestellt. Damit versuchten wir, den einleitend geschürzten Knoten in seinen wesentlichen Verwicklungen zu beleuchten. Im folgenden gilt es nun, diesen Knoten zu l?sen, wofür sich die verschiedensten, jedoch nicht in gleichem Ma?e Erfolg versprechenden Wege anboten. Wir hielten es für zweckm?作者: 細絲 時間: 2025-3-30 01:29
The Quiescent Chromospheres and Transition Regions of Active Dwarf Stars: What are We Learning from recommended for all students of economics however experienced. ‘ A.W.Coats, Kyklos ‘Professor Pheby in this much needed book gives a brilliant conducted tour ofour subject.‘ G.L.S.Shackle, foreword to the Japanese edition. Pheby has provided an antidote to the dangers of adopting, an excessively par作者: 自傳 時間: 2025-3-30 06:57 作者: 逢迎白雪 時間: 2025-3-30 09:47
The Distribution of Chromospheric Emission Strengths Among Red Dwarfsthe presumption that the willingness to attend, for example, in-service training, is related to formal qualifications and work experience, but may also be affected by the current context. The focus of this paper is to understand these relationships in the South African context, where the enhancement作者: Rebate 時間: 2025-3-30 14:41 作者: Canyon 時間: 2025-3-30 17:02
The Atmosphere of a Probably Very Young by Dra-Type Flare Star very general terms, both disciplines have the same subject matter, namely the bulk of science. Speaking in more particular terms, they still appear to coincide in their subjects: namely, particular components of science, like concepts, principles, methods, theories and research programs. Consequent作者: FECT 時間: 2025-3-30 23:52
Some Properties of Stellar Transition Regions large mammal species and general biodiversity. It covers issues of rigorous sampling, modeling, estimation and adaptive management of animal populations using cutting-edge tools, such as camera-traps, genetic identification and Geographic Information Systems (GIS), applied under the modern statisti作者: 上釉彩 時間: 2025-3-31 04:37
Quiescent Coronae of Active Chromosphere Starsole in cancer chemotherapy by catalyzing the degradation of potentially cytotoxic purine deoxynucleoside analogs, e.g., 2′-deoxy-6-thioguanosine. More recently, the identification of an immunodeficiency disorder associated with a deficiency in PNP (Giblett .., 1975) has drawn attention to this enzym作者: pacific 時間: 2025-3-31 05:33 作者: oxidant 時間: 2025-3-31 11:28 作者: NATAL 時間: 2025-3-31 15:22
phy is the most universal integrated circuit process and is of great influence in gating progress towards smallness, but other areas are of equal importance. They include device design, material deposition (epitaxial films, oxides, silicides, ..), and development of processes for transferring resist作者: impale 時間: 2025-3-31 19:51 作者: 我怕被刺穿 時間: 2025-4-1 01:36 作者: 機構 時間: 2025-4-1 04:52
0067-0057 took place during the 1979 Montreal General Assembly. We recognized that a fundamental change was taking place in the study of these objects. Space-borne instruments (especially lUE and Einstein) and a new genera- tion of ground-based equipment were having a profound effect on the range of investiga
