LEADER 03198nam 2200601 a 450 001 9910438118903321 005 20200520144314.0 010 $a1-283-63371-X 010 $a9786613946164 010 $a94-007-4295-9 024 7 $a10.1007/978-94-007-4295-6 035 $a(CKB)2670000000256387 035 $a(EBL)1030216 035 $a(OCoLC)810147476 035 $a(SSID)ssj0000739300 035 $a(PQKBManifestationID)11478276 035 $a(PQKBTitleCode)TC0000739300 035 $a(PQKBWorkID)10687064 035 $a(PQKB)10067891 035 $a(DE-He213)978-94-007-4295-6 035 $a(MiAaPQ)EBC1030216 035 $z(PPN)25886348X 035 $a(PPN)168337630 035 $a(EXLCZ)992670000000256387 100 $a20120917d2013 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aSolar history $ean introduction /$fClaudio Vita-Finzi 205 $a1st ed. 2013. 210 $aDordrecht $cSpringer$d2013 215 $a1 online resource (95 p.) 225 0$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 $aSolar activity$xHistory 607 $aSolar system$xHistory 615 0$aSolar activity$xHistory. 676 $a523.7 700 $aVita-Finzi$b Claudio$0152489 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910438118903321 996 $aSolar History$92266076 997 $aUNINA LEADER 01406nam a2200337 i 4500 001 991003290379707536 005 20241121164813.0 008 981214s1976 it er ||1 | fre d 035 $ab11138889-39ule_inst 035 $aPARLA179041$9ExL 040 $aBibl. Dip.le Aggr. Studi Umanistici - Sez. Filosofia$bita$dSocioculturale Scs 041 1 $afre$hlat 082 04$a194$223 100 1 $aArmogathe, Jean Robert$0184574 245 10$aIndex des Regulae ad directionem ingenii de Rene Descartes /$cJ.-R. Armogathe, J.-L. Marion ; avec des listes de lecons et conjectures etablies par G. Crapulli 260 $aRoma :$bEdizioni dell'Ateneo,$c1976 300 $aXXII, 163 p. ;$c24 cm. 490 1 $aCorpus Cartesianum ;$v1 490 1 $aLessico intellettuale europeo ;$v10 600 14$aDescartes, René .$tRegulae ad directionem ingenii$vSpogli lessicali 700 1 $aMarion, Jean-Luc 700 1 $aCrapulli, Giovanni 700 1 $aDescartes, René 830 0$aCorpus Cartesianum ;$v1 830 0$aLessico intellettuale europeo ;$v10 907 $a.b11138889$b23-02-17$c28-06-02 912 $a991003290379707536 945 $aLE005 194 DES01. C.C. 01$g1$i2005000030208$lle005$o-$pE0.00$q-$rl$s-$t0$u6$v1$w6$x0$y.i11278596$z28-06-02 996 $aIndex des Regulae ad directionem ingenii de Rene Descartes$9871635 997 $aUNISALENTO 998 $ale005$b01-01-98$cm$da$e-$ffre$git$h0$i1