標(biāo)題: Titlebook: Exploration of the Planetary System; A. Woszczyk,C. Iwaniszewska Book 1974 International Astronomical Union 1974 Planet.Planetary system.S [打印本頁] 作者: 管玄樂團(tuán) 時(shí)間: 2025-3-21 18:36
書目名稱Exploration of the Planetary System影響因子(影響力)
書目名稱Exploration of the Planetary System影響因子(影響力)學(xué)科排名
書目名稱Exploration of the Planetary System網(wǎng)絡(luò)公開度
書目名稱Exploration of the Planetary System網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Exploration of the Planetary System被引頻次
書目名稱Exploration of the Planetary System被引頻次學(xué)科排名
書目名稱Exploration of the Planetary System年度引用
書目名稱Exploration of the Planetary System年度引用學(xué)科排名
書目名稱Exploration of the Planetary System讀者反饋
書目名稱Exploration of the Planetary System讀者反饋學(xué)科排名
作者: 瘙癢 時(shí)間: 2025-3-21 22:22
Testosterone Metabolism in Skinns of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volatile compounds, and the ‘optical’ properties of the grain-gas medium. A summary of available and still needed basic (input) data and some currently available results are presented.作者: 時(shí)代 時(shí)間: 2025-3-22 00:27
https://doi.org/10.1007/978-3-663-07687-2rs estimate the physical cross section . (.) with respect to the geometric one .ο. Then a statistical approach for an assembly of grains gives the accretion or destruction rates for these small particles. Therefore, according to their characteristic velocities, the following processes have been studied: rupture, fusion, vaporization.作者: mercenary 時(shí)間: 2025-3-22 05:08 作者: CAPE 時(shí)間: 2025-3-22 09:16 作者: 不理會(huì) 時(shí)間: 2025-3-22 15:24 作者: 不理會(huì) 時(shí)間: 2025-3-22 19:11
Anatomie und Physiologie der Hautlution groundbased studies..These results establish that the average value over the entire disk is quite low but allows that locally larger values may exist as reported by Barker. A more complete description of this work appeared in . . (1974), 213.作者: 打算 時(shí)間: 2025-3-22 22:57
On the Growth Mechanism of Grains in a Primordial Stage of the Solar Nebulars estimate the physical cross section . (.) with respect to the geometric one .ο. Then a statistical approach for an assembly of grains gives the accretion or destruction rates for these small particles. Therefore, according to their characteristic velocities, the following processes have been studied: rupture, fusion, vaporization.作者: 下邊深陷 時(shí)間: 2025-3-23 02:23
First Results of the Soviet-Polish Space Experiment ‘Intercosmos-Kopernik 500’ta recorded. First results of the space observations are shown. The correlation between electron density of the ambient plasma, ion-sheath capacitance of the aerial, and the upper hybrid frequency can be seen.作者: 空中 時(shí)間: 2025-3-23 08:52
Profondeur de Penetration et Formation des Raies Dans une Atmosphere Diffusantene permettent d’améliorer la connaissance de la structure interne des nuages..L’application de cette méthode à l’interprétation des raies formées sur Vénus a permis de préciser que l’épaisseur optique des nuages, dans le cas du modèle de Hansen serait de l’ordre de 40 et leur sommet situé vers 60 km d’altitude.作者: Mucosa 時(shí)間: 2025-3-23 12:44
Nature of the Venus Clouds as Derived from Their Polarization particle properties deduced from the polarization eliminate all but one of the cloud compositions which have been proposed for Venus. A concentrated solution of sulfuric acid (H.SO.-H.O) provides good agreement with the polarization data.作者: cinder 時(shí)間: 2025-3-23 15:16
Water Vapor in Venus Determined by Airborne Observations of the 8200 ? Bandlution groundbased studies..These results establish that the average value over the entire disk is quite low but allows that locally larger values may exist as reported by Barker. A more complete description of this work appeared in . . (1974), 213.作者: 織物 時(shí)間: 2025-3-23 20:50
Book 1974 of his birth, came during the XIV General Assembly of IAU in Brighton. The Executive Committee has approved it in the program of the Extraordinary (Copernicus) General Assembly ofIAU in Poland in 1973. The IAU Symposium No 65 (Copernicus Symposium IV) on the ‘Exploration of the Planetary System‘ wa作者: 大都市 時(shí)間: 2025-3-24 01:20
Status of Molecular Opacities of Interest in the Modeling of a Proto-Solar Nebulans of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volatile compounds, and the ‘optical’ properties of the grain-gas medium. A summary of available and still needed basic (input) data and some currently available results are presented.作者: Inkling 時(shí)間: 2025-3-24 03:25 作者: amplitude 時(shí)間: 2025-3-24 07:40 作者: frozen-shoulder 時(shí)間: 2025-3-24 13:53 作者: intuition 時(shí)間: 2025-3-24 18:18 作者: 類人猿 時(shí)間: 2025-3-24 21:26 作者: adj憂郁的 時(shí)間: 2025-3-24 23:31
Robert W. Baloh,Robert E. BartholomewWe have searched for molecular lines in planetary atmospheres using the PEPSIOS spectrometer with an instrumental width about equal to that of the expected absorption line, and in the case of Jupiter, with the additional feature of Doppler compensation over the planetary disc.作者: 放氣 時(shí)間: 2025-3-25 03:32
Planetary FormationExisting theories of planetary formation (based on a continuous solar nebula or on discrete objects) are briefly reviewed.作者: 颶風(fēng) 時(shí)間: 2025-3-25 07:59
Numerical Modelling of the Reflection Spectrum of Venus in the Visual and Near Infrared RangesThe influence of a dense molecular atmosphere under a cloud layer on spectral albedo of a planet is investigated. The lengths of paths of protons in the clouds are calculated. Experimental spectral transmission functions were used to calculate gas absorption. The results are compared with experimental data.作者: PAGAN 時(shí)間: 2025-3-25 13:34
Interpretation of the Illumination Measurements by the Automatic Interplanetary Station ‘Venera 8’Measurements of the downward light flux during the descent from an altitude of 50 km to the ground have been made. Atmospheric layers with different optical thicknesses have been discovered. The optical properties of Venus atmosphere for different cloud models have been studied.作者: 座右銘 時(shí)間: 2025-3-25 16:16 作者: phase-2-enzyme 時(shí)間: 2025-3-25 23:22
International Astronomical Union Symposiahttp://image.papertrans.cn/e/image/319395.jpg作者: Migratory 時(shí)間: 2025-3-26 00:44 作者: vanquish 時(shí)間: 2025-3-26 06:36 作者: Hangar 時(shí)間: 2025-3-26 11:00 作者: 殘酷的地方 時(shí)間: 2025-3-26 13:56
Infrared Spectra of Venuspectroscopically forty years ago, and minor constituents (CO, HF, HCl) have been found more recently. The infrared spectra also provide a means of studying the motions of her cloudy atmosphere. The composition of the clouds has been sought in the reflection spectrum of Venus, and some of the evidence for their nature is discussed.作者: GILD 時(shí)間: 2025-3-26 18:41
978-90-277-0450-4International Astronomical Union 1974作者: 一美元 時(shí)間: 2025-3-26 23:38 作者: phlegm 時(shí)間: 2025-3-27 02:52
https://doi.org/10.1007/978-94-010-2206-4Planet; Planetary system; Solar System; Variation; astronomy; interferometry; solar; sun作者: 忘川河 時(shí)間: 2025-3-27 05:25
Testosterone Metabolism in Skinas models for the solar nebula during planet formation and for the atmospheres of some planets. Specifically considered are the equilibrium compositions of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volat作者: ineffectual 時(shí)間: 2025-3-27 12:29
https://doi.org/10.1007/978-3-663-07687-2 and electromagnetic mechanisms between grains. The velocity distribution function has been investigated for grains embedded in a turbulent gaseous medium. Results have been obtained for protoplanetary nebula densities ranging from 10. to 10. g cm.. Considering interactions between two grains, photo作者: MIME 時(shí)間: 2025-3-27 14:12
https://doi.org/10.1007/978-3-642-90940-5the Earth’s atmosphere as a medium extending to infinity, with a stationary Earth imbedded at the center. Indeed, it was this concept that led Ptolemy, among many others, to conclude that the Earth could not be moving, for otherwise it would be subject to a gale-force wind caused by its own motion. 作者: 蔓藤圖飾 時(shí)間: 2025-3-27 19:38 作者: 富饒 時(shí)間: 2025-3-27 22:19
https://doi.org/10.1007/978-3-642-81039-8. (or ..) parts of the refractive indices of water, ice, and liquid ammonia are presented graphically. Work currently in progress on solid ammonia and on sulphuric acid is discussed. Other approaches to studies of the properties of aerosols in planetary atmospheres are presented briefly.作者: Palpitation 時(shí)間: 2025-3-28 04:08 作者: 付出 時(shí)間: 2025-3-28 07:59
,Pr?vention und Schadensbegrenzung,pectroscopically forty years ago, and minor constituents (CO, HF, HCl) have been found more recently. The infrared spectra also provide a means of studying the motions of her cloudy atmosphere. The composition of the clouds has been sought in the reflection spectrum of Venus, and some of the evidenc作者: 搖曳的微光 時(shí)間: 2025-3-28 10:56 作者: 壟斷 時(shí)間: 2025-3-28 18:40 作者: 殺蟲劑 時(shí)間: 2025-3-28 22:31 作者: 樣式 時(shí)間: 2025-3-29 01:19 作者: 一起平行 時(shí)間: 2025-3-29 07:08
Diskussion der Untersuchungsergebnisse,ns in the abundance have been found with both position and time. The total two-way transmission has varied from less than 5 to 77 . of water vapor. Comparisons will be made between the water vapor abundances, presence of UV features, and the CO. abundances determined from near simultaneous observati作者: Recessive 時(shí)間: 2025-3-29 08:05
The Escape of Planetary Atmospheresbegan to take form whether or not the Moon possessed an atmosphere. And this idea was gradually extended to other planets..The lunar observers of the late eighteenth century set out to ascertain whether the Moon indeed showed visible traces of an atmosphere. In 1792, Schroter recorded what he interp作者: 有角 時(shí)間: 2025-3-29 11:38
Modern Research in High Resolution Infrared Spectroscopy and Its Importance to Planetary Physicserg done in the early 50’s are not summarized in this paper because they are all consolidated in three previous publications. On the other hand, more recent measurements on CO. are scattered in several publications and, therefore, an attempt has been made to collect them together in this article. Th作者: inspiration 時(shí)間: 2025-3-29 15:43
Ground-Based Observations of Mars and Venus Water Vapor during 1972 and 1973e Mariner 9 IRIS and Mars 3 observations made during the same period..During the second period (..= 124° to 266°) observations were made to follow the seasonal latitudinal and diurnal changes in the water vapor abundance in the Martian atmosphere. The water vapor abundance declines from a maximum of作者: 鎮(zhèn)壓 時(shí)間: 2025-3-29 21:01 作者: 琺瑯 時(shí)間: 2025-3-30 01:05 作者: Perineum 時(shí)間: 2025-3-30 06:51 作者: 微生物 時(shí)間: 2025-3-30 11:13 作者: erythema 時(shí)間: 2025-3-30 16:17
Book 1974 of the Polish Acade- my of Sciences made possible the participation of several young astronomers in this meeting. We are very grateful to Professor P. Swings, the Director of the Astrophysical Institute of the University of Liege, Belgium, for accepting the task of chairing this symposium. His expe作者: infringe 時(shí)間: 2025-3-30 17:09
1743-9213 rofessor P. Swings, the Director of the Astrophysical Institute of the University of Liege, Belgium, for accepting the task of chairing this symposium. His expe978-90-277-0450-4978-94-010-2206-4Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: 使長(zhǎng)胖 時(shí)間: 2025-3-30 23:28
Status of Molecular Opacities of Interest in the Modeling of a Proto-Solar Nebulaas models for the solar nebula during planet formation and for the atmospheres of some planets. Specifically considered are the equilibrium compositions of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volat作者: 現(xiàn)實(shí) 時(shí)間: 2025-3-31 03:04
On the Growth Mechanism of Grains in a Primordial Stage of the Solar Nebula and electromagnetic mechanisms between grains. The velocity distribution function has been investigated for grains embedded in a turbulent gaseous medium. Results have been obtained for protoplanetary nebula densities ranging from 10. to 10. g cm.. Considering interactions between two grains, photo作者: 無彈性 時(shí)間: 2025-3-31 08:14
The Escape of Planetary Atmospheresthe Earth’s atmosphere as a medium extending to infinity, with a stationary Earth imbedded at the center. Indeed, it was this concept that led Ptolemy, among many others, to conclude that the Earth could not be moving, for otherwise it would be subject to a gale-force wind caused by its own motion. 作者: –LOUS 時(shí)間: 2025-3-31 10:52 作者: gerrymander 時(shí)間: 2025-3-31 15:19 作者: averse 時(shí)間: 2025-3-31 20:19 作者: 裁決 時(shí)間: 2025-4-1 00:20
Infrared Spectra of Venuspectroscopically forty years ago, and minor constituents (CO, HF, HCl) have been found more recently. The infrared spectra also provide a means of studying the motions of her cloudy atmosphere. The composition of the clouds has been sought in the reflection spectrum of Venus, and some of the evidenc作者: Cpr951 時(shí)間: 2025-4-1 01:57
Profondeur de Penetration et Formation des Raies Dans une Atmosphere Diffusanteprofondeur de pénétration du rayonnement dans un nuage; on peut alors obtenir une information précise sur l’épaisseur optique de la couche nuageuse dans laquelle a été formée une raie spectrale. La relation qui existe entre la fréquence de la raie observée et l’altitude de la région de l’atmosphère 作者: MENT 時(shí)間: 2025-4-1 09:08 作者: 絕食 時(shí)間: 2025-4-1 13:06
