ACE Observations of the Bastille Day 2000 Interplanetary Disturbances
dc.contributor.author | Zurbuchen, Thomas H. | en_US |
dc.contributor.author | Skoug, R. M. | en_US |
dc.contributor.author | Smith, C. W. | en_US |
dc.contributor.author | Ness, N. F. | en_US |
dc.contributor.author | Burlaga, L. F. | en_US |
dc.contributor.author | McComas, D. J. | en_US |
dc.contributor.author | Gloeckler, George | en_US |
dc.contributor.author | Haggerty, D. K. | en_US |
dc.contributor.author | Gold, R. E. | en_US |
dc.contributor.author | Desai, M. I. | en_US |
dc.contributor.author | Mason, G. M. | en_US |
dc.contributor.author | Mazur, J. E. | en_US |
dc.contributor.author | Dwyer, J. R. | en_US |
dc.contributor.author | Popecki, M. A. | en_US |
dc.contributor.author | Möbius, E. | en_US |
dc.contributor.author | Cohen, C. M. S. | en_US |
dc.contributor.author | Leske, R. A. | en_US |
dc.date.accessioned | 2006-09-11T13:44:04Z | |
dc.date.available | 2006-09-11T13:44:04Z | |
dc.date.issued | 2001-12 | en_US |
dc.identifier.citation | Smith, C.W.; Ness, N.F.; Burlaga, L.F.; Skoug, R.M.; McComas, D.J.; Zurbuchen, T.H.; Gloeckler, G.; Haggerty, D.K.; Gold, R.E.; Desai, M.I.; Mason, G.M.; Mazur, J.E.; Dwyer, J.R.; Popecki, M.A.; Möbius, E.; Cohen, C.M.S.; Leske, R.A.; (2001). "ACE Observations of the Bastille Day 2000 Interplanetary Disturbances." Solar Physics 204 (1-2): 227-252. <http://hdl.handle.net/2027.42/43716> | en_US |
dc.identifier.issn | 0038-0938 | en_US |
dc.identifier.issn | 1573-093X | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/43716 | |
dc.description.abstract | We present ACE observations for the six-day period encompassing the Bastille Day 2000 solar activity. A high level of transient activity at 1 AU, including ICME-driven shocks, magnetic clouds, shock-accelerated energetic particle populations, and solar energetic ions and electrons, are described. We present thermal ion composition signatures for ICMEs and magnetic clouds from which we derive electron temperatures at the source of the disturbances and we describe additional enhancements in some ion species that are clearly related to the transient source. We describe shock acceleration of 0.3–2.0 MeV nucl −1 protons and minor ions and the relative inability of some of the shocks to accelerate significant energetic ion populations near 1 AU. We report the characteristics of < 20 MeV nucl −1 solar energetic ions and < 0.32 MeV electrons and attempt to relate the release of energetic electrons to particular source regions. | en_US |
dc.format.extent | 398750 bytes | |
dc.format.extent | 3115 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Kluwer Academic Publishers; Springer Science+Business Media | en_US |
dc.subject.other | Astrophysics | en_US |
dc.subject.other | Physics | en_US |
dc.title | ACE Observations of the Bastille Day 2000 Interplanetary Disturbances | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Atmospheric, Oceanic and Space Sciences | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, USA | en_US |
dc.contributor.affiliationum | Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, USA | en_US |
dc.contributor.affiliationother | Bartol Research Institute, University of Delaware, Newark, Delaware, 19716, U.S.A | en_US |
dc.contributor.affiliationother | Bartol Research Institute, University of Delaware, Newark, Delaware, 19716, U.S.A | en_US |
dc.contributor.affiliationother | Code 692, NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, U.S.A | en_US |
dc.contributor.affiliationother | Los Alamos National Laboratory, Los Alamos, NM, 87545, U.S.A | en_US |
dc.contributor.affiliationother | Space Science and Engineering Division, Southwest Research Institute, P.O. Drawer 28510 | en_US |
dc.contributor.affiliationother | Applied Physics Laboratory, Johns Hopkins University, 11100, Johns Hopkins Road, Laurel | en_US |
dc.contributor.affiliationother | Applied Physics Laboratory, Johns Hopkins University, 11100, Johns Hopkins Road, Laurel | en_US |
dc.contributor.affiliationother | Department of Physics, University of Maryland, College Park, MD, U.S.A | en_US |
dc.contributor.affiliationother | Aerospace Corporation, El Segundo, CA, 90245-4691, U.S.A | en_US |
dc.contributor.affiliationother | Institute for the Study of Earth, Oceans and Space, University of New Hampshire, Durham | en_US |
dc.contributor.affiliationother | California Institute of Technology, Pasadena, CA, 91125, U.S.A | en_US |
dc.contributor.affiliationother | California Institute of Technology, Pasadena, CA, 91125, U.S.A | en_US |
dc.contributor.affiliationother | Institute for the Study of Earth, Oceans and Space, University of New Hampshire, Durham | en_US |
dc.contributor.affiliationother | Florida Institute of Technology, Melbourne, FL, 32901, U.S.A | en_US |
dc.contributor.affiliationother | Department of Physics, University of Maryland, College Park, MD, U.S.A | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/43716/1/11207_2004_Article_380058.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1023/A:1014265108171 | en_US |
dc.identifier.source | Solar Physics | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
Remediation of Harmful Language
The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.
Accessibility
If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.