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001 978-3-319-24151-7
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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