標題: Titlebook: Cartography of the Sun and the Stars; Jean-Pierre Rozelot,Coralie Neiner Book 2016 Springer International Publishing Switzerland 2016 CHAR [打印本頁] 作者: ergonomics 時間: 2025-3-21 19:23
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書目名稱Cartography of the Sun and the Stars網(wǎng)絡公開度學科排名
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書目名稱Cartography of the Sun and the Stars讀者反饋
書目名稱Cartography of the Sun and the Stars讀者反饋學科排名
作者: 刪除 時間: 2025-3-21 22:17
https://doi.org/10.1007/978-1-349-01327-2esented. Finally, I briefly dwell upon subtleties of different models that are developed for understanding both the thermal and magnetic field structures of the solar surface and subsurface respectively.作者: 漫不經(jīng)心 時間: 2025-3-22 04:09
Imaging Surface Spots from Space-Borne Photometry,f its host star is also briefly described. In all the cases, the main emphasis is on the basic principles of the modelling techniques and on their testing rather than on the results obtained from their application.作者: 分開如此和諧 時間: 2025-3-22 07:12 作者: 披肩 時間: 2025-3-22 09:24 作者: 隱語 時間: 2025-3-22 16:18
The Concession Gained and Lost, 1914–15 in early-type stars. We also discuss an extension of Doppler imaging to the problem of recovering vector distributions of stellar magnetic fields from spectropolarimetric observations and review applications of this Zeeman Doppler imaging technique in the context of stellar magnetism studies.作者: 隱語 時間: 2025-3-22 18:35 作者: Ambulatory 時間: 2025-3-23 00:54 作者: 窗簾等 時間: 2025-3-23 05:19 作者: incredulity 時間: 2025-3-23 06:03
0075-8450 equired for mapping the surface of stars.Highlights techniquThe mapping of the surface of stars requires diverse skills, analysis techniques and advanced modeling, i.e. the collaboration of scientists in various specialties. This volume gives insights into new techniques allowing for the first time 作者: BACLE 時間: 2025-3-23 12:15
Book 2016by connecting the differential rotation to the underlying physical parameters derived from helioseismology. Recent measurements of flattening of the solar surface by SDO showed that the Sun’s shape is linked to the rotation of the core. It is shown how such a result is generalizable to the stars.作者: 敲詐 時間: 2025-3-23 17:03 作者: conjunctivitis 時間: 2025-3-23 21:28
Oppositions of Religious Doctrinesnetic activity. The latitudinal variations of the meridional circulation speed, which are probably related to the large-scale converging flows, are mostly confined in shallow subsurface layers. Therefore, these variations do not necessarily affect the magnetic flux transport. The North-South asymmet作者: 引起痛苦 時間: 2025-3-24 01:50
https://doi.org/10.1007/978-1-349-02079-9es of stellar surfaces. I then present the issue of aperture synthesis with a small number of telescopes, a signature of optical/infrared interferometers compared to the radio domain. Despite the impossibility to measure the phase of visibilities because of turbulence I show that useful information 作者: agnostic 時間: 2025-3-24 04:17
The Concession Gained and Lost, 1914–15) allows to go beyond the spatial resolution limit of interferometers in order to measure angular sizes of stars, otherwise not measurable by classical OLBI techniques. The results presented here are based on ESO-VLTI interferometric observations of the Be star Achernar.作者: 松軟無力 時間: 2025-3-24 07:59 作者: 縮減了 時間: 2025-3-24 14:14 作者: 確定無疑 時間: 2025-3-24 18:25 作者: Oscillate 時間: 2025-3-24 22:11
Interferometric Surface Mapping of Rapidly Rotating Stars: Application to the Be star Achernar,) allows to go beyond the spatial resolution limit of interferometers in order to measure angular sizes of stars, otherwise not measurable by classical OLBI techniques. The results presented here are based on ESO-VLTI interferometric observations of the Be star Achernar.作者: neutrophils 時間: 2025-3-25 00:29 作者: Irrigate 時間: 2025-3-25 04:28 作者: Flu表流動 時間: 2025-3-25 08:35
978-3-319-24149-4Springer International Publishing Switzerland 2016作者: 繼承人 時間: 2025-3-25 14:30 作者: fulmination 時間: 2025-3-25 18:49 作者: Negligible 時間: 2025-3-25 21:43
https://doi.org/10.1007/978-1-349-01327-2e stars as can be derived from their wide-band optical light curves. Spot modelling is becoming more and more important thanks to the high-precision, high duty-cycle photometric time series made available by space-borne telescopes designed to search for planets through the method of transits. I revi作者: STALL 時間: 2025-3-26 02:25 作者: 作嘔 時間: 2025-3-26 06:39 作者: 聯(lián)合 時間: 2025-3-26 12:01
Outdoor Recreation Activities and Needs,lication of long-baseline interferometry to the determination of the photospheric shape of fast rotating stars. I present the example of the VLT Interferometer observations of the nearby Be star Achernar (.?Eri), using the VINCI (two telescopes) and PIONIER (four telescopes) beam combiners. I presen作者: DEMN 時間: 2025-3-26 14:32
https://doi.org/10.1007/978-1-349-02079-9k of Michelson at the end of the XIXth—beginning of the XXth when he first resolved the surface of a star, Betelgeuse, with his colleague Pease. Images were obtained for the first time 20 years ago with the COAST instrument and interferometers have made constant progress to reach the minimum level w作者: 下船 時間: 2025-3-26 20:14
The Concession Gained and Lost, 1914–15st rotation velocities and thus those for which the consequences of rotation are the strongest. On the stellar photosphere fast-rotation induces (1) a geometrical flattening and (2) a non-uniform distribution of flux/effective temperature (gravity darkening effect). A detailed mapping of these effec作者: 蔓藤圖飾 時間: 2025-3-26 21:34 作者: Spinal-Tap 時間: 2025-3-27 04:52
Cartography of the Sun and the Stars978-3-319-24151-7Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 熔巖 時間: 2025-3-27 07:26
Economics of Outdoor Recreation,l of Espinosa Lara and Rieutord (Astron Astrophys 533:A43, 2011), which gives the gravity darkening in early-type stars. I also discuss the problem of deriving gravity darkening in stars owning a convective envelope and in those that are members of a binary system.作者: conservative 時間: 2025-3-27 10:02
Jean-Pierre Rozelot,Coralie NeinerPresents insights into how to image and map the surface of stars.Covers a diverse set of skills, analysis techniques and advanced modeling required for mapping the surface of stars.Highlights techniqu作者: BARK 時間: 2025-3-27 16:56
Lecture Notes in Physicshttp://image.papertrans.cn/c/image/222220.jpg作者: archaeology 時間: 2025-3-27 20:19
Physical Processes Leading to Surface Inhomogeneities: The Case of Rotation,l of Espinosa Lara and Rieutord (Astron Astrophys 533:A43, 2011), which gives the gravity darkening in early-type stars. I also discuss the problem of deriving gravity darkening in stars owning a convective envelope and in those that are members of a binary system.作者: 沒血色 時間: 2025-3-27 22:05
Reconstructing Images in Astrophysics, an Inverse Problem Point of View,he rest of the chapter focuses on the resolution of the inverse problem. In the general form, the observed image is given by a Fredholm integral containing the object and the response of the instrument. Its inversion is formulated using a linear algebra. The discretized object and image of size . × 作者: finale 時間: 2025-3-28 04:47 作者: 威脅你 時間: 2025-3-28 07:50 作者: d-limonene 時間: 2025-3-28 13:47
Reconstruction of Thermal and Magnetic Field Structure of the Solar Subsurface Through Helioseismol calculations and modeling of magnetic field structure. Recent discovery of Sun’s oscillations whose amplitudes and frequencies are estimated with an unprecedented precision heralded a new era in solar physics that unraveled the hitherto unknown mysteries of the Sun’s thermal and magnetic field stru作者: 蠟燭 時間: 2025-3-28 15:14
Physical Processes Leading to Surface Inhomogeneities: The Case of Rotation,l of Espinosa Lara and Rieutord (Astron Astrophys 533:A43, 2011), which gives the gravity darkening in early-type stars. I also discuss the problem of deriving gravity darkening in stars owning a convective envelope and in those that are members of a binary system.作者: lipoatrophy 時間: 2025-3-28 22:48
Interferometry to Determine Stellar Shapes: Application to Achernar,lication of long-baseline interferometry to the determination of the photospheric shape of fast rotating stars. I present the example of the VLT Interferometer observations of the nearby Be star Achernar (.?Eri), using the VINCI (two telescopes) and PIONIER (four telescopes) beam combiners. I presen作者: 受人支配 時間: 2025-3-28 23:39
Interferometry to Image Surface Spots,k of Michelson at the end of the XIXth—beginning of the XXth when he first resolved the surface of a star, Betelgeuse, with his colleague Pease. Images were obtained for the first time 20 years ago with the COAST instrument and interferometers have made constant progress to reach the minimum level w