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Titlebook: Cartography of the Sun and the Stars; Jean-Pierre Rozelot,Coralie Neiner Book 2016 Springer International Publishing Switzerland 2016 CHAR

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樓主: ergonomics
31#
發(fā)表于 2025-3-26 21:34:15 | 只看該作者
32#
發(fā)表于 2025-3-27 04:52:56 | 只看該作者
Cartography of the Sun and the Stars978-3-319-24151-7Series ISSN 0075-8450 Series E-ISSN 1616-6361
33#
發(fā)表于 2025-3-27 07:26:18 | 只看該作者
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.
34#
發(fā)表于 2025-3-27 10:02:23 | 只看該作者
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
35#
發(fā)表于 2025-3-27 16:56:33 | 只看該作者
Lecture Notes in Physicshttp://image.papertrans.cn/c/image/222220.jpg
36#
發(fā)表于 2025-3-27 20:19:10 | 只看該作者
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.
37#
發(fā)表于 2025-3-27 22:05:48 | 只看該作者
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 . ×
38#
發(fā)表于 2025-3-28 04:47:19 | 只看該作者
39#
發(fā)表于 2025-3-28 07:50:24 | 只看該作者
40#
發(fā)表于 2025-3-28 13:47:06 | 只看該作者
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
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