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Cometary charge exchange diagnostics in UV and X‐ray
dc.contributor.authorBodewits, D.en_US
dc.contributor.authorChristian, D.J.en_US
dc.contributor.authorCarter, J.A.en_US
dc.contributor.authorDennerl, K.en_US
dc.contributor.authorEwing, I.en_US
dc.contributor.authorHoekstra, R.en_US
dc.contributor.authorLepri, S.T.en_US
dc.contributor.authorLisse, C.M.en_US
dc.contributor.authorWolk, S.J.en_US
dc.date.accessioned2012-05-21T15:47:48Z
dc.date.available2013-06-11T19:15:51Zen_US
dc.date.issued2012-04en_US
dc.identifier.citationBodewits, D.; Christian, D.J.; Carter, J.A.; Dennerl, K.; Ewing, I.; Hoekstra, R.; Lepri, S.T.; Lisse, C.M.; Wolk, S.J. (2012). "Cometary charge exchange diagnostics in UV and X‐ray." Astronomische Nachrichten 333(4): 335-340. <http://hdl.handle.net/2027.42/91138>en_US
dc.identifier.issn0004-6337en_US
dc.identifier.issn1521-3994en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/91138
dc.description.abstractSince the initial discovery of cometary charge exchange emission, more than 20 comets have been observed with a variety of X‐ray and UV observatories. This observational sample offers a broad variety of comets, solar wind environments and observational conditions. It clearly demonstrates that solar wind charge exchange emission provides a wealth of diagnostics, which are visible as spatial, temporal, and spectral emission features. We review the possibilities and limitations of each of those in this contribution (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)en_US
dc.publisherWILEY‐VCH Verlagen_US
dc.subject.otherAtomic Processesen_US
dc.subject.otherComets: Generalen_US
dc.subject.otherRadiation Mechanism: Non‐Thermalen_US
dc.subject.otherSolar Winden_US
dc.titleCometary charge exchange diagnostics in UV and X‐rayen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumThe University of Michigan, Ann Arbor, MI 48109‐2143, USAen_US
dc.contributor.affiliationotherMax‐Planck‐Institut für extraterrestrische Physik, Gießenbachstraße, D‐85748 Garching, Germanyen_US
dc.contributor.affiliationotherDepartment of Physics and Astronomy, University of Leicester, Leicester, LE1 1RH, UKen_US
dc.contributor.affiliationotherDept. of Astronomy, University of Maryland, College Park, MD 20742‐2421, USAen_US
dc.contributor.affiliationotherDepartment of Physics and Astronomy, California State University, 18111 Nordhoff Street, Northridge, CA 91330, USAen_US
dc.contributor.affiliationotherDept. of Astronomy, University of Maryland, College Park, MD 20742‐2421, USAen_US
dc.contributor.affiliationotherHarvard‐Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USAen_US
dc.contributor.affiliationotherPlanetary Exploration Group, Space Department, JHU‐APL, 11100 Johns Hopkins Rd, Laurel, MD 20723, USAen_US
dc.contributor.affiliationotherKVI Atomic Physics, University of Groningen, Zernikelaan 25, NL‐9747 AA Groningen, The Netherlandsen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/91138/1/335_ftp.pdf
dc.identifier.doi10.1002/asna.201211659en_US
dc.identifier.sourceAstronomische Nachrichtenen_US
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dc.owningcollnameInterdisciplinary and Peer-Reviewed


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