Search

Your search keyword '"Haggerty, D.K."' showing total 15 results
Start Over Author "Haggerty, D.K."
15 results on '"Haggerty, D.K."'

5. Io's Effect on Energetic Charged Particles as Seen in Juno Data

Author

Paranicas, C., primary, Mauk, B.H., additional, Haggerty, D.K., additional, Clark, G., additional, Kollmann, P., additional, Rymer, A.M., additional, Westlake, J., additional, Allen, R.C., additional, Szalay, J., additional, Ebert, R.W., additional, Sulaiman, A.H., additional, Imai, M., additional, Roussos, E., additional, Krupp, N., additional, Nénon, Q., additional, Bagenal, F., additional, and Bolton, S. J., additional

Published
2019
Full Text
View/download PDF

10. Energetic particles in the jovian magnetotail

Author

McNutt, R.L., Jr., Haggerty, D.K., Hill, M.E., Krimigis, S.M., Livi, S., Ho, G.C., Gurnee, R.S., Mauk, B.H., Mitchell, D.G., Roelof, E.C., McComas, D.J., Bagenal, F., Elliott, H.A., Brown, L.E., Kusterer, M., Vandegriff, J., Stern, S.A., Weaver, H.A., Spencer, J.R., and Moore, J.M.

Subjects
Solar wind -- Influence, Jupiter (Planet) -- Observations, Jupiter (Planet) -- Magnetic properties, Jupiter (Planet) -- Thermal properties, Satellites -- Jupiter, Satellites -- Magnetic properties, Satellites -- Thermal properties, New Horizons (Space probe) -- Services
Published
2007

11. ACE Observations of the Bastille Day 2000 Interplanetary Disturbances

Author

Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, USA, Bartol Research Institute, University of Delaware, Newark, Delaware, 19716, U.S.A, Code 692, NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, U.S.A, Los Alamos National Laboratory, Los Alamos, NM, 87545, U.S.A, Space Science and Engineering Division, Southwest Research Institute, P.O. Drawer 28510, Applied Physics Laboratory, Johns Hopkins University, 11100, Johns Hopkins Road, Laurel, Department of Physics, University of Maryland, College Park, MD, U.S.A, Aerospace Corporation, El Segundo, CA, 90245-4691, U.S.A, Institute for the Study of Earth, Oceans and Space, University of New Hampshire, Durham, California Institute of Technology, Pasadena, CA, 91125, U.S.A, Florida Institute of Technology, Melbourne, FL, 32901, U.S.A, Ann Arbor, Zurbuchen, Thomas H., Skoug, R.M., Smith, C.W., Ness, N.F., Burlaga, L.F., McComas, D.J., Gloeckler, George, 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., Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, USA, Bartol Research Institute, University of Delaware, Newark, Delaware, 19716, U.S.A, Code 692, NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, U.S.A, Los Alamos National Laboratory, Los Alamos, NM, 87545, U.S.A, Space Science and Engineering Division, Southwest Research Institute, P.O. Drawer 28510, Applied Physics Laboratory, Johns Hopkins University, 11100, Johns Hopkins Road, Laurel, Department of Physics, University of Maryland, College Park, MD, U.S.A, Aerospace Corporation, El Segundo, CA, 90245-4691, U.S.A, Institute for the Study of Earth, Oceans and Space, University of New Hampshire, Durham, California Institute of Technology, Pasadena, CA, 91125, U.S.A, Florida Institute of Technology, Melbourne, FL, 32901, U.S.A, Ann Arbor, Zurbuchen, Thomas H., Skoug, R.M., Smith, C.W., Ness, N.F., Burlaga, L.F., McComas, D.J., Gloeckler, George, 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., and Leske, R.A.

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.

Published
2006

12. Observations of the longitudinal spread of solar energetic particle events in solar cycle 24

Author

Cohen, C.M.S., primary, Mason, G.M., additional, Wiedenbeck, M.E., additional, Haggerty, D.K., additional, Gomez-Herrero, R., additional, Christian, E. R., additional, Cummings, A.C., additional, Korth, A., additional, Labrador, A. W., additional, Leske, R.A., additional, Mall, U., additional, Mewaldt, R.A., additional, Stone, E.C., additional, and Rosenvinge, T.T. Von, additional

Published
2012
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results