標(biāo)題: Titlebook: Characterizing Stellar and Exoplanetary Environments; Helmut Lammer,Maxim Khodachenko Book 2015 The Editor(s) (if applicable) and The Auth [打印本頁] 作者: 皺紋 時(shí)間: 2025-3-21 19:41
書目名稱Characterizing Stellar and Exoplanetary Environments影響因子(影響力)
書目名稱Characterizing Stellar and Exoplanetary Environments影響因子(影響力)學(xué)科排名
書目名稱Characterizing Stellar and Exoplanetary Environments網(wǎng)絡(luò)公開度
書目名稱Characterizing Stellar and Exoplanetary Environments網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Characterizing Stellar and Exoplanetary Environments被引頻次
書目名稱Characterizing Stellar and Exoplanetary Environments被引頻次學(xué)科排名
書目名稱Characterizing Stellar and Exoplanetary Environments年度引用
書目名稱Characterizing Stellar and Exoplanetary Environments年度引用學(xué)科排名
書目名稱Characterizing Stellar and Exoplanetary Environments讀者反饋
書目名稱Characterizing Stellar and Exoplanetary Environments讀者反饋學(xué)科排名
作者: GAVEL 時(shí)間: 2025-3-21 22:46
Exoplanet Host Star Radiation and Plasma Environmenttmosphere depends on the evolution of its host star. We summarize the available techniques for measuring or estimating the X-ray, EUV, and UV radiation of host stars with different spectral types and ages.作者: 小隔間 時(shí)間: 2025-3-22 00:37 作者: 狂熱文化 時(shí)間: 2025-3-22 05:54 作者: 就職 時(shí)間: 2025-3-22 11:59
Stellar Driven Evolution of Hydrogen-Dominated Atmospheres from Earth-Like to Super-Earth-Type Exoplicant importance for planets with relatively weak Jeans-type escape or heavier particles (e.g., O, C, N). From the diversity of non-thermal escape mechanisms, in the present chapter we focus on ion pick-up and discuss the importance of other loss mechanisms. The general conclusion of the chapter is,作者: 鍍金 時(shí)間: 2025-3-22 15:14 作者: 鍍金 時(shí)間: 2025-3-22 19:06 作者: CAB 時(shí)間: 2025-3-22 23:50 作者: 鋼筆尖 時(shí)間: 2025-3-23 04:21 作者: Arthropathy 時(shí)間: 2025-3-23 09:31
0067-0057 vironments, exoplanet upper atmosphere and environment observations, exoplanet and stellar magnetospheres, and exoplanet observation and characterization. The book closes with an outlook on the future of this r978-3-319-37936-4978-3-319-09749-7Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: DEVIL 時(shí)間: 2025-3-23 13:15 作者: 上釉彩 時(shí)間: 2025-3-23 15:26
https://doi.org/10.1007/978-3-8348-9468-7tions, discussed in this Chapter, show that the gaseous envelopes around hot Jupiters may be significantly non-spherical and, at the same time, stationary and long-lived. These results are of fundamental importance for the interpretation of observational data.作者: charisma 時(shí)間: 2025-3-23 19:16
,Fertigteile mit Ortbetonerg?nzung,sphere of a hydrogen-rich exoplanet. Partial deposition rates of the stellar XUV radiation due to the photolytic processes in the . transition region in the upper atmosphere of HD 209458b were calculated. The Monte Carlo model developed by authors was used to calculate the collisional kinetics and t作者: RALES 時(shí)間: 2025-3-24 01:26 作者: 搖晃 時(shí)間: 2025-3-24 03:17
,Fertigteile mit Ortbetonerg?nzung,es have claimed that stars with close-in, massive exoplanets are statistically more active, but others conclude that this correlation is just the product of a selection bias. Studies with the Kepler-satellite show that superflares exist, but they do not seem to be caused by the interaction between s作者: 尖牙 時(shí)間: 2025-3-24 07:39 作者: 梯田 時(shí)間: 2025-3-24 13:04
Physikalisch-technisches Grundwissen, limited. For the next decade, the post-HST era, the World Space Observatory UltraViolet (WSO–UV) will be the only large telescope class mission for UV observations, both spectroscopic and imaging. In its potential, the WSO–UV mission is similar to the HST, but all the observing time will be availab作者: FIS 時(shí)間: 2025-3-24 16:42
Helmut Lammer,Maxim KhodachenkoPresents studies of exoplanets under extreme stellar radiation and plasma conditions.Analyzes findings from Hubble Space Telescope observations of transiting exoplanets.Presents applications of advanc作者: Employee 時(shí)間: 2025-3-24 19:18 作者: 不透明 時(shí)間: 2025-3-25 00:49 作者: 無可爭辯 時(shí)間: 2025-3-25 03:52 作者: 陰謀小團(tuán)體 時(shí)間: 2025-3-25 11:02 作者: 記成螞蟻 時(shí)間: 2025-3-25 14:10
Ground-Based Exoplanet Projectsready so large that it is not possible discussing them adequately in just one article. I will therefor just outline what the new concepts are, and mention only a few examples that demonstrate what the new instruments will offer to us.作者: Facet-Joints 時(shí)間: 2025-3-25 18:28
https://doi.org/10.1007/978-3-319-09749-7CoRoT Space Observatory; Exoplanet Atmospheres; Exoplanet Environment; Exoplanet Observations; Exoplanet作者: Organonitrile 時(shí)間: 2025-3-25 23:04
978-3-319-37936-4The Editor(s) (if applicable) and The Author(s) 2015作者: 懶惰民族 時(shí)間: 2025-3-26 03:29 作者: 束以馬具 時(shí)間: 2025-3-26 05:26
,Fertigteile mit Ortbetonerg?nzung,dge of how they evolve with time. Determining this empirically requires the ability to study the winds of stars of various ages and activity levels, but this is not easy to do as the coronal winds of solar-like stars are very hard to detect. Relevant observations are here reviewed, as well as more t作者: CRAFT 時(shí)間: 2025-3-26 11:54 作者: 打擊 時(shí)間: 2025-3-26 14:27 作者: 傻瓜 時(shí)間: 2025-3-26 18:49
https://doi.org/10.1007/978-3-8348-9468-7 objects. Since they are so close to the host stars, their atmospheres form and evolve under the action of very active gas dynamical processes caused by the gravitational field and irradiation of the host star. As a matter of fact, the atmospheres of several of these planets fill their Roche lobes, 作者: novelty 時(shí)間: 2025-3-26 21:00 作者: depreciate 時(shí)間: 2025-3-27 03:53 作者: 出汗 時(shí)間: 2025-3-27 07:26 作者: Harpoon 時(shí)間: 2025-3-27 11:30 作者: 平息 時(shí)間: 2025-3-27 14:11 作者: 厭倦嗎你 時(shí)間: 2025-3-27 17:56 作者: amputation 時(shí)間: 2025-3-28 00:52
https://doi.org/10.1007/978-3-540-78592-7 In this paper we discuss a role of Alfvén radius for different types of magnetospheres and magnetosphere-disk systems. Among the astrophysical disks considered here are the magnetic disks surrounding the outer planets in the Solar System (Jupiter and Saturn) and exoplanets, the heliospheric current作者: 無脊椎 時(shí)間: 2025-3-28 04:33 作者: 聯(lián)合 時(shí)間: 2025-3-28 08:32 作者: 敲竹杠 時(shí)間: 2025-3-28 12:46 作者: 冬眠 時(shí)間: 2025-3-28 16:19 作者: 分開如此和諧 時(shí)間: 2025-3-28 21:37
,Fertigteile mit Ortbetonerg?nzung,dge of how they evolve with time. Determining this empirically requires the ability to study the winds of stars of various ages and activity levels, but this is not easy to do as the coronal winds of solar-like stars are very hard to detect. Relevant observations are here reviewed, as well as more theoretical methods of addressing the problem.作者: 先兆 時(shí)間: 2025-3-29 00:59 作者: 憂傷 時(shí)間: 2025-3-29 04:51
,Tragf?higkeit schlanker Druckglieder, both more pronounced in the near-UV and starts at an earlier time than the optical lightcurve. These features of the near-UV transit of WASP-12b have intrigued several modellers. In this Chapter, we review the different interpretations of the near-UV observations of the system.作者: CYN 時(shí)間: 2025-3-29 11:04 作者: Engaged 時(shí)間: 2025-3-29 12:25 作者: 細(xì)胞膜 時(shí)間: 2025-3-29 19:27
0067-0057 ons of transiting exoplanets.Presents applications of advanc.In this book an international group of specialists discusses studies of exoplanets subjected to extreme stellar radiation and plasma conditions. It is shown that such studies will help us to understand how terrestrial planets and their atm作者: infringe 時(shí)間: 2025-3-29 20:54
Living with Stars: Future Space-Based Exoplanet Search and Characterization Missionsthe real sense of the term, i.e. a direct comparison, both between objects outside the Solar System, as well as with objects within our home system. In this chapter we describe briefly all the space assets that are either in orbit, intended to be launched within the near future and also those that are decided for the intermediate time perspective.作者: extract 時(shí)間: 2025-3-30 03:09
Book 2015s shown that such studies will help us to understand how terrestrial planets and their atmospheres, including the early Venus, Earth and Mars, evolved during the host star’s active early phase. The book presents an analysis of findings from Hubble Space Telescope observations of transiting exoplanet作者: obnoxious 時(shí)間: 2025-3-30 07:04
https://doi.org/10.1007/978-3-8348-9468-7esulting influence on surrounding planets – in more and more detail. Here we review what is known about the magnetic fields of cool stars, covering relevant techniques such as Zeeman Doppler Imaging (ZDI), field extrapolation and wind simulations, as well as relevant observational results.作者: 本土 時(shí)間: 2025-3-30 08:47 作者: Leaven 時(shí)間: 2025-3-30 13:56
Energierechtliche Rahmenbedingungen,he different ways in which a planetary magnetic field may modify the planetary evolution and reviews the different methods that have been suggested to detect these fields. These methods are compared and we evaluate which techniques have the highest potential for future detection of exoplanetary magnetic fields.作者: 錢財(cái) 時(shí)間: 2025-3-30 18:57 作者: Dislocation 時(shí)間: 2025-3-31 00:31
Detection Methods and Relevance of Exoplanetary Magnetic Fieldshe different ways in which a planetary magnetic field may modify the planetary evolution and reviews the different methods that have been suggested to detect these fields. These methods are compared and we evaluate which techniques have the highest potential for future detection of exoplanetary magnetic fields.作者: 生氣的邊緣 時(shí)間: 2025-3-31 03:09
Alfvén Radius: A Key Parameter for Astrophysical Magnetospheresf its origin, direction of motion and material in it) in the presence of a strong magnetic field is located close to the Alfvén radius. For magnetized planets a concept of Alfvén radius is important as for the interaction with the solar/stellar wind, either for the inter-magnetospheric processes.作者: Ballad 時(shí)間: 2025-3-31 05:39 作者: FELON 時(shí)間: 2025-3-31 11:58
Stellar Winds in Timedge of how they evolve with time. Determining this empirically requires the ability to study the winds of stars of various ages and activity levels, but this is not easy to do as the coronal winds of solar-like stars are very hard to detect. Relevant observations are here reviewed, as well as more t作者: 經(jīng)典 時(shí)間: 2025-3-31 17:26 作者: 殺人 時(shí)間: 2025-3-31 20:51 作者: 飾帶 時(shí)間: 2025-3-31 23:52 作者: Gastric 時(shí)間: 2025-4-1 04:02 作者: ungainly 時(shí)間: 2025-4-1 06:26
Stellar Driven Evolution of Hydrogen-Dominated Atmospheres from Earth-Like to Super-Earth-Type Exoplnet atmospheres. We focus mainly on planets within the Earth- to super-Earth mass domain and consider both, thermal and nonthermal atmospheric escape processes. The type of thermal loss mechanism depends on the so-called escape parameter, which is the ratio of the gravitational energy of a particle
