LEADER 01651nam 2200337Ia 450 001 996389332403316 005 20221108081306.0 035 $a(CKB)1000000000646578 035 $a(EEBO)2248534337 035 $a(OCoLC)9923108700971 035 $a(EXLCZ)991000000000646578 100 $a20061013d1553 uy 0 101 0 $aeng 135 $aurbn||||a|bb| 200 00$aAnno III. & IIII. Edvvardi sexti$b[electronic resource] $eActes made in the session of this present parlament, holden vpon prorogation at Westminster, the .iiii daie of Nouembre, in the thirde yere of the reigne of our most dread souuereine Lorde Edward the .vi by the grace of God, king of Englande, Fraunce, and Ireland, defendour of the faith, and of the Churche of Englande, and also of Irelande, in earth the supreme head: and there continued, and kept to the first daie of Februarie, in the .iiii. yere of the reigne of our saied Souuereine Lorde, as foloweth 210 $aImprinted at London $cby Richard Graston [i.e. R. Tottell], printer to the Kynges Maiestie.$d[1553, i.e. 1560?] 215 $axxxij leaves 300 $aImprint from colophon. 300 $aReproduction of the original in the Harvard University. Library. 330 $aeebo-0018 606 $aLaw$zEngland$vSources$vEarly works to 1800 606 $aSession laws$zEngland$vEarly works to 1800 607 $aGreat Britain$xHistory$yEdward VI, 1547-1553$vSources$vEarly works to 1800 615 0$aLaw 615 0$aSession laws 801 0$bUMI 801 1$bUMI 906 $aBOOK 912 $a996389332403316 996 $aAnno III. & IIII. Edvvardi sexti$92397608 997 $aUNISA LEADER 01006nam a2200265 i 4500 001 991002109469707536 005 20020508190640.0 008 950606s1994 it ||| | ita 020 $a8817843113 035 $ab10960697-39ule_inst 035 $aPARLA154688$9ExL 040 $aDip.to Scienze pedagogiche$bita 100 1 $aPapert, Seymour$045647 245 12$aI bambini e il computer :$bnuove idee per i nuovi strumenti dell'educazione /$cSeymour Papert 260 $aMilano :$bRCS Rizzoli Libri & Grandi Opere,$c1994 300 $a253 p. ;$c21 cm. 650 4$aApprendimento e tecnologia 650 4$aComputer$xUtilizzazione didattica 650 4$aTecnologie educativo-didattiche 907 $a.b10960697$b21-09-06$c28-06-02 912 $a991002109469707536 945 $aLE022 MP 124 F 39$g1$i2022000116190$lle022$o-$pE0.00$q-$rl$s- $t0$u19$v5$w19$x0$y.i11070092$z28-06-02 996 $aBambini e il computer$9863894 997 $aUNISALENTO 998 $ale022$b01-01-95$cm$da $e-$fita$git $h2$i1 LEADER 03260nam 22005295 450 001 9910163006203321 005 20250609111723.0 010 $a3-319-50989-6 024 7 $a10.1007/978-3-319-50989-1 035 $a(CKB)3710000001041343 035 $a(DE-He213)978-3-319-50989-1 035 $a(MiAaPQ)EBC4791274 035 $a(PPN)198338759 035 $a(MiAaPQ)EBC6241998 035 $a(EXLCZ)993710000001041343 100 $a20170125d2017 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aDifferential Rotation in Sun-like Stars from Surface Variability and Asteroseismology /$fby Martin Bo Nielsen 205 $a1st ed. 2017. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2017. 215 $a1 online resource (XVI, 101 p. 29 illus., 18 illus. in color.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 311 08$a3-319-50988-8 320 $aIncludes bibliographical references and index. 327 $aIntroduction -- Rotation Periods of 12 000 Main-sequence Kepler Stars -- Rotational Splitting as a Function of Mode Frequency for Six Sunlike Stars -- Constraining Differential Rotation of Sun-like Stars from Asteroseismic and Starspot Rotation Periods -- Discussion: Constraining Interior Rotational Shear -- Appendices. 330 $aIn his PhD dissertation Martin Bo Nielsen performs observational studies of rotation in stars like the Sun. The interior rotation in stars is thought to be one of the driving mechanisms of stellar magnetic activity, but until now this mechanism was unconstrained by observational data. NASA?s Kepler space mission provides high-precision observations of Sun-like stars which allow rotation to be inferred using two independent methods: asteroseismology measures the rotation of the stellar interior, while the brightness variability caused by features on the stellar surface trace the rotation of its outermost layers. By combining these two techniques Martin Bo Nielsen was able to place upper limits on the variation of rotation with depth in five Sun-like stars. These results suggest that the interior of other Sun-like stars also rotate in much the same way as our own Sun. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstrophysics 606 $aAstronomy$vObservations 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$aAstronomy 615 0$aAstronomy?Observations. 615 14$aAstrophysics and Astroparticles. 615 24$aAstronomy, Observations and Techniques. 676 $a523.01 700 $aNielsen$b Martin Bo$4aut$4http://id.loc.gov/vocabulary/relators/aut$0819532 906 $aBOOK 912 $a9910163006203321 996 $aDifferential Rotation in Sun-like Stars from Surface Variability and Asteroseismology$91826385 997 $aUNINA