LEADER 04203nam 22006615 450 001 996466814103316 005 20200706133224.0 010 $a3-319-24151-6 024 7 $a10.1007/978-3-319-24151-7 035 $a(CKB)3710000000627441 035 $a(SSID)ssj0001657291 035 $a(PQKBManifestationID)16438496 035 $a(PQKBTitleCode)TC0001657291 035 $a(PQKBWorkID)14986890 035 $a(PQKB)10276192 035 $a(DE-He213)978-3-319-24151-7 035 $a(MiAaPQ)EBC5587414 035 $a(Au-PeEL)EBL5587414 035 $a(OCoLC)944444915 035 $z(PPN)258846461 035 $a(PPN)192769375 035 $a(EXLCZ)993710000000627441 100 $a20160311d2016 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 10$aCartography of the Sun and the Stars$b[electronic resource] /$fedited by Jean-Pierre Rozelot, Coralie Neiner 205 $a1st ed. 2016. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2016. 215 $a1 online resource (X, 206 p. 78 illus., 48 illus. in color.) 225 1 $aLecture Notes in Physics,$x0075-8450 ;$v914 300 $aBibliographic Level Mode of Issuance: Monograph 311 $a3-319-24149-4 327 $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. 330 $aThe mapping of the surface of stars requires diverse skills, analysis techniques and advanced modeling, i.e. the collaboration of scientists in various specialties. This volume gives insights into new techniques allowing for the first time to obtain resolved images of stars. It takes stock of what has been achieved so far in Chile, on the ESO VLTI instrument or, in the States, on the CHARA instrument. In recent times interferometry, combined with adaptive optics has allowed to reconstruct images of stars. Besides the Sun (of course) by now five stars have been resolved in detail. In addition to interferometry, this book highlights techniques used for mapping the surfaces of stars using photometry made by space observatories; Zeeman- and Doppler Imaging; mapping the surface element abundances via spectroscopy. This book will also take stock of the best images of the solar surface, made by connecting the differential rotation to the underlying physical parameters derived from helioseismology. Recent measurements of flattening of the solar surface by SDO showed that the Sun?s shape is linked to the rotation of the core. It is shown how such a result is generalizable to the stars. 410 0$aLecture Notes in Physics,$x0075-8450 ;$v914 606 $aAstrophysics 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 615 0$aAstrophysics. 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 14$aAstrophysics and Astroparticles. 615 24$aAstronomy, Observations and Techniques. 676 $a523.01 702 $aRozelot$b Jean-Pierre$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aNeiner$b Coralie$4edt$4http://id.loc.gov/vocabulary/relators/edt 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a996466814103316 996 $aCartography of the Sun and the Stars$92174077 997 $aUNISA