派博傳思國際中心

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
書目名稱Cartography of the Sun and the Stars影響因子(影響力)




書目名稱Cartography of the Sun and the Stars影響因子(影響力)學科排名




書目名稱Cartography of the Sun and the Stars網(wǎng)絡公開度




書目名稱Cartography of the Sun and the Stars網(wǎng)絡公開度學科排名




書目名稱Cartography of the Sun and the Stars被引頻次




書目名稱Cartography of the Sun and the Stars被引頻次學科排名




書目名稱Cartography of the Sun and the Stars年度引用




書目名稱Cartography of the Sun and the Stars年度引用學科排名




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




歡迎光臨 派博傳思國際中心 (http://www.pjsxioz.cn/) Powered by Discuz! X3.5
金塔县| 肇庆市| 图们市| 府谷县| 甘肃省| 历史| 承德市| 彰化市| 新疆| 淮北市| 邻水| 将乐县| 牙克石市| 永昌县| 来安县| 平泉县| 上饶县| 永年县| 潍坊市| 绵阳市| 大宁县| 石阡县| 睢宁县| 碌曲县| 苍南县| 图片| 兰溪市| 兰考县| 元谋县| 广河县| 闸北区| 靖西县| 志丹县| 民丰县| 丽江市| 岗巴县| 韩城市| 赫章县| 石台县| 东港市| 阿坝|