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010   $a9786613946164
010   $a94-007-4295-9
024 7 $a10.1007/978-94-007-4295-6
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035   $a(DE-He213)978-94-007-4295-6
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100   $a20120904d2013      u|             0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 10$aSolar History$b[electronic resource] $eAn Introduction /$fby Claudio Vita-Finzi
205   $a1st ed. 2013.
210  1$aDordrecht :$cSpringer Netherlands :$cImprint: Springer,$d2013.
215   $a1 online resource (95 p.)
225 1 $aSpringerBriefs in Astronomy,$x2191-9100
300   $aDescription based upon print version of record.
311   $a94-007-4294-0 
320   $aIncludes bibliographical references and index.
327   $aPreface -- 1. Introduction -- 2. Origins.- 3. The young Sun.- 4. Isotopes and ice cores -- 5. Cosmogenic radiocarbon -- 6. The solar cycle.- 7. Solar  rotation -- 8. Contemporary history -- 9. The Lessons of History -- Index.
330   $aBeyond the four centuries of sunspot observation and the five decades during which artificial satellites have monitored the Sun ? that is to say for 99.99999% of the Sun?s existence ? our knowledge of solar history depends largely on analogy with kindred main sequence stars, on the outcome of various kinds of modelling, and on indirect measures of solar activity. They include the analysis of lunar rocks and meteorites for evidence of solar flares and other components of the solar cosmic-ray (SCR) flux, and the measurement of cosmogenic isotopes in wood, stratified ice and marine sediments to evaluate changes in the galactic cosmic-ray (GCR) flux and thus infer changes in the sheltering magnetic fields of the solar wind. In addition, shifts in the global atmospheric circulation which appear to result from cyclic fluctuations in solar irradiance have left their mark in river sediments and in the isotopic composition of cave deposits. In this volume the results these sources have already produced have been summarised, paying special attention to those that reflect processes in different parts of the Sun?s interior and that display periodicities and trends which may enable us to forecast future large-scale environmental changes.
410  0$aSpringerBriefs in Astronomy,$x2191-9100
606   $aAstronomy
606   $aAstrophysics
606   $aAtmospheric sciences
606   $aGeophysics
606   $aPlanetology
606   $aAstronomy, Astrophysics and Cosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22006
606   $aAtmospheric Sciences$3https://scigraph.springernature.com/ontologies/product-market-codes/G36000
606   $aGeophysics and Environmental Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P32000
606   $aPlanetology$3https://scigraph.springernature.com/ontologies/product-market-codes/G18010
607   $aSun$xEvolution
615  0$aAstronomy.
615  0$aAstrophysics.
615  0$aAtmospheric sciences.
615  0$aGeophysics.
615  0$aPlanetology.
615 14$aAstronomy, Astrophysics and Cosmology.
615 24$aAtmospheric Sciences.
615 24$aGeophysics and Environmental Physics.
615 24$aPlanetology.
676   $a523.7
700   $aVita-Finzi$b Claudio$4aut$4http://id.loc.gov/vocabulary/relators/aut$0152489
906   $aBOOK
912   $a9910438118903321
996   $aSolar History$92266076
997   $aUNINA