000 | 03710nam a22004695i 4500 | ||
---|---|---|---|
001 | 978-3-319-24151-7 | ||
003 | DE-He213 | ||
005 | 20190213151311.0 | ||
007 | cr nn 008mamaa | ||
008 | 160311s2016 gw | s |||| 0|eng d | ||
020 |
_a9783319241517 _9978-3-319-24151-7 |
||
024 | 7 |
_a10.1007/978-3-319-24151-7 _2doi |
|
050 | 4 | _aQB460-466 | |
072 | 7 |
_aPHVB _2bicssc |
|
072 | 7 |
_aSCI005000 _2bisacsh |
|
072 | 7 |
_aPHVB _2thema |
|
082 | 0 | 4 |
_a523.01 _223 |
245 | 1 | 0 |
_aCartography of the Sun and the Stars _h[electronic resource] / _cedited by Jean-Pierre Rozelot, Coralie Neiner. |
250 | _a1st ed. 2016. | ||
264 | 1 |
_aCham : _bSpringer International Publishing : _bImprint: Springer, _c2016. |
|
300 |
_aX, 206 p. 78 illus., 48 illus. in color. _bonline resource. |
||
336 |
_atext _btxt _2rdacontent |
||
337 |
_acomputer _bc _2rdamedia |
||
338 |
_aonline resource _bcr _2rdacarrier |
||
347 |
_atext file _bPDF _2rda |
||
490 | 1 |
_aLecture Notes in Physics, _x0075-8450 ; _v914 |
|
505 | 0 | _aPreface -- Reconstructing images in astrophysics, an inverse problem point of view -- Reconstruction of the solar subsurface through helioseismology with SDO -- Imaging surface spots from space-borne photometry -- Reconstruction of Thermal and Magnetic Field Structure of the Solar Subsurface through Helioseismology -- Physical processes leading to surface inhomogeneities: the case of rotation -- Interferometry to determine stellar shapes: application to Achernar -- Interferometry to image surface spots -- Interferometric Surface Mapping of RapidlyRotating Stars. - Application to the Be star Achernar -- Doppler and Zeeman Doppler Imaging of Stars. | |
520 | _aThe 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 to obtain resolved images of stars. It takes stock of what has been achieved so far in Chile, on the ESO VLTI instrument or, in the States, on the CHARA instrument. In recent times interferometry, combined with adaptive optics has allowed to reconstruct images of stars. Besides the Sun (of course) by now five stars have been resolved in detail. In addition to interferometry, this book highlights techniques used for mapping the surfaces of stars using photometry made by space observatories; Zeeman- and Doppler Imaging; mapping the surface element abundances via spectroscopy. This book will also take stock of the best images of the solar surface, made by 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. | ||
650 | 1 | 4 |
_aAstrophysics and Astroparticles. _0http://scigraph.springernature.com/things/product-market-codes/P22022 |
650 | 2 | 4 |
_aAstronomy, Observations and Techniques. _0http://scigraph.springernature.com/things/product-market-codes/P22014 |
700 | 1 |
_aRozelot, Jean-Pierre. _eeditor. _4edt _4http://id.loc.gov/vocabulary/relators/edt |
|
700 | 1 |
_aNeiner, Coralie. _eeditor. _4edt _4http://id.loc.gov/vocabulary/relators/edt |
|
710 | 2 | _aSpringerLink (Online service) | |
773 | 0 | _tSpringer eBooks | |
776 | 0 | 8 |
_iPrinted edition: _z9783319241494 |
776 | 0 | 8 |
_iPrinted edition: _z9783319241500 |
830 | 0 |
_aLecture Notes in Physics, _x0075-8450 ; _v914 |
|
856 | 4 | 0 | _uhttps://doi.org/10.1007/978-3-319-24151-7 |
912 | _aZDB-2-PHA | ||
912 | _aZDB-2-LNP | ||
999 |
_c10201 _d10201 |