Solar wind charge exchange and local hot bubble X‐ray emission with the DXL sounding rocket experiment
dc.contributor.author | Galeazzi, M. | en_US |
dc.contributor.author | Collier, M.R. | en_US |
dc.contributor.author | Cravens, T. | en_US |
dc.contributor.author | Koutroumpa, D. | en_US |
dc.contributor.author | Kuntz, K.D. | en_US |
dc.contributor.author | Lepri, S. | en_US |
dc.contributor.author | McCammon, D. | en_US |
dc.contributor.author | Porter, F. S. | en_US |
dc.contributor.author | Prasai, K. | en_US |
dc.contributor.author | Robertson, I. | en_US |
dc.contributor.author | Snowden, S. | en_US |
dc.contributor.author | Thomas, N.E. | en_US |
dc.contributor.author | Uprety, Y. | en_US |
dc.date.accessioned | 2012-05-21T15:46:55Z | |
dc.date.available | 2013-06-11T19:15:46Z | en_US |
dc.date.issued | 2012-04 | en_US |
dc.identifier.citation | Galeazzi, M.; Collier, M.R.; Cravens, T.; Koutroumpa, D.; Kuntz, K.D.; Lepri, S.; McCammon, D.; Porter, F. S.; Prasai, K.; Robertson, I.; Snowden, S.; Thomas, N.E.; Uprety, Y. (2012). "Solar wind charge exchange and local hot bubble X‐ray emission with the DXL sounding rocket experiment." Astronomische Nachrichten 333(4): 383-387. <http://hdl.handle.net/2027.42/91104> | en_US |
dc.identifier.issn | 0004-6337 | en_US |
dc.identifier.issn | 1521-3994 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/91104 | |
dc.description.abstract | The Diffuse X‐ray emission from the Local Galaxy (DXL) sounding rocket is a NASA approved mission with a scheduled first launch in December 2012. Its goal is to identify and separate the X‐ray emission of the solar wind charge exchange (SWCX) from that of the local hot bubble (LHB) to improve our understanding of both. To separate the SWCX contribution from the LHB, DXL will use the SWCX signature due to the helium focusing cone at l = 185°, b = –18°. DXL uses large area proportional counters, with an area of 1000 cm 2 and grasp of about 10 cm 2 sr both in the 1/4 and 3/4 keV bands. Thanks to the large grasp, DXL will achieve in a 5‐minute flight what cannot be achieved by current and future X‐ray satellites (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) | en_US |
dc.publisher | WILEY‐VCH Verlag | en_US |
dc.subject.other | ISM: Bubbles | en_US |
dc.subject.other | Instrumentation: Detectors | en_US |
dc.subject.other | X‐Rays: ISM | en_US |
dc.subject.other | Solar Wind | en_US |
dc.subject.other | Interplanetary Medium | en_US |
dc.title | Solar wind charge exchange and local hot bubble X‐ray emission with the DXL sounding rocket experiment | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | University of Michigan, 2455 Hayward St., Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationother | University of Wisconsin, Department of Physics, 1150 University Ave., Madison, WI 53706, USA | en_US |
dc.contributor.affiliationother | University of Miami, Department of Physics, 1320 Campo Sano Dr., Coral Gables, FL 33146, USA | en_US |
dc.contributor.affiliationother | NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA | en_US |
dc.contributor.affiliationother | University of Kansas, Department of Physics and Astronomy, 1251 Wescoe Hall Dr., Lawrence, KS 66045, USA | en_US |
dc.contributor.affiliationother | LATMOS‐IPSL/CNRS, 11 Boulevard d'Alembert, 78280 Guyancourt, France | en_US |
dc.contributor.affiliationother | The Johns Hopkins University, The Henry A. Rowland Department of Physics and Astronomy, Baltimore, MD 21218, USA | en_US |
dc.contributor.affiliationother | Correspondence | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/91104/1/383_ftp.pdf | |
dc.identifier.doi | 10.1002/asna.201211665 | en_US |
dc.identifier.source | Astronomische Nachrichten | en_US |
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dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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