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Scientific objectives and capabilities of the Coronal Solar Magnetism Observatory
dc.contributor.authorTomczyk, S.
dc.contributor.authorLandi, E.
dc.contributor.authorBurkepile, J. T.
dc.contributor.authorCasini, R.
dc.contributor.authorDeLuca, E. E.
dc.contributor.authorFan, Y.
dc.contributor.authorGibson, S. E.
dc.contributor.authorLin, H.
dc.contributor.authorMcIntosh, S. W.
dc.contributor.authorSolomon, S. C.
dc.contributor.authorToma, G.
dc.contributor.authorWijn, A. G.
dc.contributor.authorZhang, J.
dc.date.accessioned2016-10-17T21:19:52Z
dc.date.available2017-10-05T14:33:49Zen
dc.date.issued2016-08
dc.identifier.citationTomczyk, S.; Landi, E.; Burkepile, J. T.; Casini, R.; DeLuca, E. E.; Fan, Y.; Gibson, S. E.; Lin, H.; McIntosh, S. W.; Solomon, S. C.; Toma, G.; Wijn, A. G.; Zhang, J. (2016). "Scientific objectives and capabilities of the Coronal Solar Magnetism Observatory." Journal of Geophysical Research: Space Physics 121(8): 7470-7487.
dc.identifier.issn2169-9380
dc.identifier.issn2169-9402
dc.identifier.urihttps://hdl.handle.net/2027.42/134244
dc.description.abstractMagnetic influences increase in importance in the solar atmosphere from the photosphere out into the corona, yet our ability to routinely measure magnetic fields in the outer solar atmosphere is lacking. We describe the scientific objectives and capabilities of the COronal Solar Magnetism Observatory (COSMO), a proposed synoptic facility designed to measure magnetic fields and plasma properties in the large‐scale solar atmosphere. COSMO comprises a suite of three instruments chosen to enable the study of the solar atmosphere as a coupled system: (1) a coronagraph with a 1.5 m aperture to measure the magnetic field, temperature, density, and dynamics of the corona; (2) an instrument for diagnostics of chromospheric and prominence magnetic fields and plasma properties; and (3) a white light K‐coronagraph to measure the density structure and dynamics of the corona and coronal mass ejections. COSMO will provide a unique combination of magnetic field, density, temperature, and velocity observations in the corona and chromosphere that have the potential to transform our understanding of fundamental physical processes in the solar atmosphere and their role in the origins of solar variability and space weather.Key PointsSociety is becoming increasingly vulnerable to the effects of space weatherThe physical processes responsible for solar activity remain poorly understoodCOSMO will provide key measurements to advance our understanding of solar processes and activity
dc.publisherWiley Periodicals, Inc.
dc.publisherSpringer
dc.subject.othersolar corona
dc.titleScientific objectives and capabilities of the Coronal Solar Magnetism Observatory
dc.typeArticleen_US
dc.rights.robotsIndexNoFollow
dc.subject.hlbsecondlevelAstronomy and Astrophysics
dc.subject.hlbtoplevelScience
dc.description.peerreviewedPeer Reviewed
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/134244/1/jgra52783_am.pdf
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/134244/2/jgra52783.pdf
dc.identifier.doi10.1002/2016JA022871
dc.identifier.sourceJournal of Geophysical Research: Space Physics
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