LEADER 04340nam 2200577 450 001 9910468030203321 005 20200520144314.0 010 $a2-7598-2196-X 024 7 $a10.1051/978-2-7598-2196-9 035 $a(CKB)4340000000265179 035 $a(MiAaPQ)EBC5349377 035 $a(PPN)233404031 035 $a(Au-PeEL)EBL5349377 035 $a(CaPaEBR)ebr11545392 035 $a(OCoLC)1032726008 035 $a(DE-B1597)573381 035 $a(DE-B1597)9782759821969 035 $a(MiAaPQ)EBC6810258 035 $a(Au-PeEL)EBL6810258 035 $a(OCoLC)1287136911 035 $a(EXLCZ)994340000000265179 100 $a20180519d2018 uy 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 00$aVariability of the sun and sun-like stars $efrom asteroseismology to space weather /$fJ. -P Rozelot and E. S. Babayev, (eds) 210 1$aLes Ulis :$cEDP Sciences,$d[2018] 210 4$dİ2018 215 $a1 online resource (238 pages) 225 0 $aEDP Sciences Proceedings 311 $a2-7598-2195-1 327 $tFrontmatter -- $tPreface -- $tTable of contents -- $tSection 1. Solar Physics -- $tHelioseismology in Uzbekistan: past and present -- $tLocal Helioseismology of Emerging Active Region: A Case Study -- $tRealistic Simulations of Stellar Radiative MHD -- $tAdvances in Realistic MHD Simulations of the Sun and Stars -- $tA brief history of the solar diameter measurements: a critical quality assessment of the existing data -- $tSolar sunspot-forming activity and its development on the reliable Wolf numbers series -- $tWave instabilities in an anisotropic magnetized space plasma -- $tSection 2. From Helioseismology to Asteroseismology -- $tAsteroseismology with solar-like oscillations -- $tSection 3. Cosmic rays and space weather -- $tCosmic Rays and other Space Weather Phenomena Influenced on Satellites Operation, Technologies, Biosphere and People Health -- $tCosmic Rays and other Space Phenomena Dangerous for the Earth's Civilization: Beginning Steps for Founding Cosmic Ray Warning System -- $tSpace Weather Effects on Human Health -- $tSection 4. Impact of the Sun on Earth climatology -- $tCosmic Rays and other Space Phenomena Influenced on the Earth's Climate -- $tDoes climatic changes could have destroyed great civilizations? -- $tInfluence of orbital forcing and solar activity on climate change in the past 330 $aThis book is based on contributions presented at the first International Conference on Solar Physics which was organized in Baku, Azerbaijan in July 06?08, 2015, by the Science Development Foundation under the President of the Republic of Azerbaijan. The primary goals were to highlight specific aspects of modern solar physics research, including observation and theory that span from the interior of the Sun out into the wider heliosphere, as well as solar-terrestrial physics and particularly, sun-like stars. The Sun is a variable star. However, we are still far from fully understanding what and how causes this variability. Why does the Sun continue to go on, on a rhythmic scale, the so-called solar cycle, without damping? How to better understand the complicated relationships between the Sun, the heliosphere and the many proxies of long-term solar activity? How the data could be fully exploited for a better understanding of solar changes on the longest possible time scales? How our knowledge on the Sun can be transfer to other stars? What are the impacts on our terrestrial environment? These questions shape the architecture of the book. It will be of interest and useful to scientists and graduate level readers who would like to better master such up-to-date topics. 410 0$aEDP Sciences Proceedings Ser. 606 $aAstroseismology$vCongresses 607 $aSun$vCongresses 608 $aElectronic books. 615 0$aAstroseismology 676 $a523.7 700 $aRozelot$b Jean-Pierre, $4aut$4http://id.loc.gov/vocabulary/relators/aut$067603 702 $aRozelot$b J. -P 702 $aBabayev$b E. S. 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910468030203321 996 $aVariability of the sun and sun-like stars$92444459 997 $aUNINA