Cosmic rays interstellar medium theirenvironment CRISM-2011宇宙射线及其 星际介质 2011年的环境.pdf

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1、Cosmicrays&theirinterstellarmediumenvironmentCRISM-2011Sunday26June2011-Friday01July2011Montpellier,FranceRecueildesrésumésContentsAMarkovChainMonteCarlotechniquetosampletransportandsourceparametersofGalacticcosmicrays....................................1AnewnearbyPWNoverlappingtheVelaJrSNR........

2、...............1AGILEobservationsofmiddle-agedSNRs...........................1AlfvenWaveAmplificationandSelf-ContainmentofCosmic-RaysEscapingfromaSuper-novaRemnant........................................2AnIntegralViewofShocks:VIMOS-IFUObservationsofSN1006.............2CRescapefromSupernovaremnants

3、andtheirradiativesignatures............2Contribution...........................................3Contribution...........................................3Contribution...........................................3Contribution...........................................3Contribution.......................

4、....................3Contribution...........................................3CosmicRayTransportintheHeliosphereanditsConnectiontotheLocalInterstellarSpec-tra..............................................3CosmicRayproductionofBerylliumandBoronathighredshift..............4Cosmicraydrivengalacticmagne

5、ticfielddynamo......................4Cosmicraydrivengalacticwinds...............................4Cosmicrayproductionandgamma-rayemissionfromTycho’ssupernovaremnant...5Cosmicraypropagationintheinterstellarmedium.....................5Cosmicraystreaminginstabilitiesinthelong-wavelengthlimit...........

6、...5Cosmicray-inducedcarbonisotopefractionationofmoleculesindensedarkgas.....6Cosmicraysandclimateforcing................................6Cosmicraysandthethermalinstability............................6iiiCosmic-rayionisationofmolecularclouds..........................7Cosmic-rayionizationandchemistr

7、y:observations.....................7Cosmic-rayionizationandchemistry:theory........................7DiffuseGalacticGammaRaysatintermediateandhighLatitudes,ConstraintsonISMprop-ertiesandDM...................