標(biāo)題: Titlebook: Handbook of Exoplanets ; Hans J. Deeg,Juan Antonio Belmonte Living reference work 20250th edition Exoplanet search.Growth of exobiology.A [打印本頁(yè)] 作者: McKinley 時(shí)間: 2025-3-21 19:26
書(shū)目名稱(chēng)Handbook of Exoplanets 影響因子(影響力)
書(shū)目名稱(chēng)Handbook of Exoplanets 影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Handbook of Exoplanets 網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Handbook of Exoplanets 網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Handbook of Exoplanets 被引頻次
書(shū)目名稱(chēng)Handbook of Exoplanets 被引頻次學(xué)科排名
書(shū)目名稱(chēng)Handbook of Exoplanets 年度引用
書(shū)目名稱(chēng)Handbook of Exoplanets 年度引用學(xué)科排名
書(shū)目名稱(chēng)Handbook of Exoplanets 讀者反饋
書(shū)目名稱(chēng)Handbook of Exoplanets 讀者反饋學(xué)科排名
作者: 浪費(fèi)時(shí)間 時(shí)間: 2025-3-22 00:15 作者: ALLEY 時(shí)間: 2025-3-22 02:13 作者: WAG 時(shí)間: 2025-3-22 04:59 作者: 外形 時(shí)間: 2025-3-22 11:27
Zeitgestaltung im Alltag ?lterer Menschenformed at the same time, the challenge is to determine the stellar age. Asteroseismology provides precise age determination, but in many cases the required detailed pulsation observations are not available. Here we concentrate on other techniques, which may have broader applicability but also seriou作者: outset 時(shí)間: 2025-3-22 15:57 作者: 腐蝕 時(shí)間: 2025-3-22 18:36 作者: 鋪?zhàn)?nbsp; 時(shí)間: 2025-3-23 00:05 作者: foppish 時(shí)間: 2025-3-23 02:03
https://doi.org/10.1007/978-3-662-24668-9ibing their general circulation, the most relevant atmospheric phenomena, and the models developed so far to explain their atmospheric dynamics. Observations show that these two types of fluid and cold planets differ in their general circulation at cloud level. Jupiter and Saturn are dominated by a 作者: Apraxia 時(shí)間: 2025-3-23 07:23
https://doi.org/10.1007/978-3-663-05596-9 be termed “terrestrial.” These atmospheres have much in common, in having circulations that are driven primarily by heating from the Sun and radiative cooling to space, which vary markedly with latitude. The principal response to this forcing is typically in the form of a (roughly zonally symmetric作者: 使苦惱 時(shí)間: 2025-3-23 11:41
https://doi.org/10.1007/978-3-662-68726-0rties include the chemical compositions, temperature profiles, clouds/hazes, and energy circulation. These properties, in turn, can provide key insights into the atmospheric physicochemical processes of exoplanets as well as their formation mechanisms. Major advancements in atmospheric retrieval hav作者: Esalate 時(shí)間: 2025-3-23 14:42 作者: Legend 時(shí)間: 2025-3-23 18:16 作者: 紀(jì)念 時(shí)間: 2025-3-24 00:42 作者: 無(wú)彈性 時(shí)間: 2025-3-24 02:41
https://doi.org/10.1007/978-3-658-14967-3 namely, Teide 1 (Rebolo et al. Nature 377:129–131, 1995), many searches for substellar objects have been carried out in young stellar clusters and associations, such as Pleiades, Orion, Upper Scorpius, Taurus, Chamaeleon, . Persei, Hyades, or Praesepe. The lithium test has proven to be a very usefu作者: adulterant 時(shí)間: 2025-3-24 07:34
https://doi.org/10.1007/978-3-658-36919-4hese observables can be used to deduce physical characteristics of the planet such as its averaged dayside emission, departures from uniform disk illumination, or a precise measurement of the orbital eccentricity. This technique became a reality in 2005; in this chapter we describe the basics of the作者: 思考才皺眉 時(shí)間: 2025-3-24 12:39 作者: ALIEN 時(shí)間: 2025-3-24 18:54 作者: NOVA 時(shí)間: 2025-3-24 19:40 作者: duplicate 時(shí)間: 2025-3-24 23:32
https://doi.org/10.1007/978-3-663-01820-9density, surface effective temperature, distance, and age. In this chapter, a number of basic properties for exoplanets are listed, and their dependence on fundamental stellar properties is discussed. The exoplanets with the most accurate properties are those that are transiting, where we have detec作者: agglomerate 時(shí)間: 2025-3-25 05:48 作者: narcotic 時(shí)間: 2025-3-25 09:42 作者: TRUST 時(shí)間: 2025-3-25 14:09 作者: 誹謗 時(shí)間: 2025-3-25 19:33 作者: athlete’s-foot 時(shí)間: 2025-3-25 21:26
Ages for Exoplanet Host Stars,formed at the same time, the challenge is to determine the stellar age. Asteroseismology provides precise age determination, but in many cases the required detailed pulsation observations are not available. Here we concentrate on other techniques, which may have broader applicability but also seriou作者: catagen 時(shí)間: 2025-3-26 00:36
Assessing the Interior Structure of Terrestrial Exoplanets with Implications for Habitability,understand planetary diversity and further determine how unique, or not, Earth is. Assessing interior structure is challenging because there are few data and large uncertainties. Thus, for a given exoplanet, a range of interior structure models can satisfy available data. Typically, interior models 作者: 仇恨 時(shí)間: 2025-3-26 06:50 作者: Glaci冰 時(shí)間: 2025-3-26 11:40
Atmospheric Biosignatures,lt of photosynthetic activity. Additionally, bacteria emit greenhouse gases such as methane and nitrous oxide into the atmosphere, and vegetation can emit a variety of organic molecules. In an exoplanetary context, it is important to consider whether such gas-phase species – so-called atmospheric bi作者: 引導(dǎo) 時(shí)間: 2025-3-26 15:59 作者: 蘑菇 時(shí)間: 2025-3-26 17:55
Atmospheric Dynamics of Terrestrial Planets, be termed “terrestrial.” These atmospheres have much in common, in having circulations that are driven primarily by heating from the Sun and radiative cooling to space, which vary markedly with latitude. The principal response to this forcing is typically in the form of a (roughly zonally symmetric作者: CHART 時(shí)間: 2025-3-26 23:09 作者: 胰島素 時(shí)間: 2025-3-27 03:23 作者: 禍害隱伏 時(shí)間: 2025-3-27 06:01
Biosignature False Positives,extrasolar planets – we must infer the presence of life from its impact on the local or global environment. These “biosignatures,” often identified from the known influence of terrestrial organisms on the Earth’s atmosphere and surface, could be misdiagnosed when we apply them to alien worlds. The s作者: glucagon 時(shí)間: 2025-3-27 12:44 作者: convulsion 時(shí)間: 2025-3-27 16:15 作者: 拾落穗 時(shí)間: 2025-3-27 18:15
Characterization of Exoplanets: Secondary Eclipses,hese observables can be used to deduce physical characteristics of the planet such as its averaged dayside emission, departures from uniform disk illumination, or a precise measurement of the orbital eccentricity. This technique became a reality in 2005; in this chapter we describe the basics of the作者: 不規(guī)則的跳動(dòng) 時(shí)間: 2025-3-27 22:55 作者: Ophthalmoscope 時(shí)間: 2025-3-28 02:46
Characterizing Exoplanet Habitability,ential, as performing a census of Earthlike planets that may or may not have life will inform our understanding of how frequently life originates and is sustained on worlds other than our own. Observational techniques like high-contrast imaging and transit spectroscopy can reveal key indicators of h作者: 偏見(jiàn) 時(shí)間: 2025-3-28 07:15
Characterizing Host Stars using Asteroseismology, characterize exoplanet host stars and as a consequence also the exoplanets themselves. This synergy between asteroseismology and exoplanet science has flourished in large part due to space missions such as ., which have provided high-quality data that can be used for both types of studies. Perhaps 作者: 馬具 時(shí)間: 2025-3-28 11:10 作者: notification 時(shí)間: 2025-3-28 18:04 作者: motor-unit 時(shí)間: 2025-3-28 19:47 作者: hermitage 時(shí)間: 2025-3-29 01:00
https://doi.org/10.1007/978-3-663-12460-3atures, then introduce potential false positives for these signals, and finally discuss methods to discriminate between the two using current and future detection technologies. We conclude that it is the astrobiology community’s responsibility to thoroughly exhaust all possibilities before we resort to “l(fā)ife” as an explanation.作者: Obsequious 時(shí)間: 2025-3-29 03:44
https://doi.org/10.1007/978-3-663-05477-1ate into precise planetary radii, but asteroseismology has also proven useful in constraining eccentricities of exoplanets as well as the dynamical architecture of planetary systems. In this chapter, we introduce some basic principles of asteroseismology and review current synergies between the two fields.作者: ABOUT 時(shí)間: 2025-3-29 08:15 作者: Somber 時(shí)間: 2025-3-29 14:16
Astrometry as an Exoplanet Discovery Method,her discovery methods. The importance of stability and precision of the astrometric measurements over a long period may explain the relative lack of results, but the advent of a space mission like Gaia will certainly change the impact of astrometry in the exoplanet field.作者: 笨拙的你 時(shí)間: 2025-3-29 18:30
Biosignature False Positives,atures, then introduce potential false positives for these signals, and finally discuss methods to discriminate between the two using current and future detection technologies. We conclude that it is the astrobiology community’s responsibility to thoroughly exhaust all possibilities before we resort to “l(fā)ife” as an explanation.作者: IOTA 時(shí)間: 2025-3-29 21:42
Characterizing Host Stars using Asteroseismology,ate into precise planetary radii, but asteroseismology has also proven useful in constraining eccentricities of exoplanets as well as the dynamical architecture of planetary systems. In this chapter, we introduce some basic principles of asteroseismology and review current synergies between the two fields.作者: Excise 時(shí)間: 2025-3-30 02:08 作者: 使痛苦 時(shí)間: 2025-3-30 06:25 作者: Pudendal-Nerve 時(shí)間: 2025-3-30 11:07 作者: 敬禮 時(shí)間: 2025-3-30 16:23
https://doi.org/10.1007/978-3-658-26834-3 and discs, dynamical ejection of stellar embryos, and photoerosion. The primary contenders would seem to be turbulent fragmentation and disc fragmentation, and the observations needed to evaluate their relative importance may soon be available.作者: 山崩 時(shí)間: 2025-3-30 17:11
https://doi.org/10.1007/978-3-658-36919-4 technique, its main results in the last 12 years, and the prospects for the years to come. This chapter includes a table with references to all published detections of secondary eclipses until December 2017.作者: 諷刺滑稽戲劇 時(shí)間: 2025-3-30 21:14 作者: 性學(xué)院 時(shí)間: 2025-3-31 01:33 作者: CUR 時(shí)間: 2025-3-31 05:59
Ages for Exoplanet Host Stars,s limitations. Further development of this area requires improvements in our understanding of the evolution of stars and their age-dependent characteristics, combined with observations that allow reliable calibration of the various techniques.作者: Breach 時(shí)間: 2025-3-31 11:21
Brown Dwarf Formation: Theory, and discs, dynamical ejection of stellar embryos, and photoerosion. The primary contenders would seem to be turbulent fragmentation and disc fragmentation, and the observations needed to evaluate their relative importance may soon be available.作者: 無(wú)能性 時(shí)間: 2025-3-31 17:17 作者: 爭(zhēng)吵加 時(shí)間: 2025-3-31 17:38 作者: CHAR 時(shí)間: 2025-4-1 00:16 作者: anatomical 時(shí)間: 2025-4-1 02:07 作者: PHAG 時(shí)間: 2025-4-1 08:25
https://doi.org/10.1007/978-3-663-11903-6terogeneous observations. This chapter offers a brief introduction to Bayesian inference in the context of exoplanet research, with focus on time series analysis, and finishes with an overview of a set of freely available programming libraries.
