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Fine jet structure of electrically charged grains in Enceladus' plume

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Zeitschriftentitel: Geophysical Research Letters
Personen und Körperschaften: Jones, G. H., Arridge, C. S., Coates, A. J., Lewis, G. R., Kanani, S., Wellbrock, A., Young, D. T., Crary, F. J., Tokar, R. L., Wilson, R. J., Hill, T. W., Johnson, R. E., Mitchell, D. G., Schmidt, J., Kempf, S., Beckmann, U., Russell, C. T., Jia, Y. D., Dougherty, M. K., Waite, J. H., Magee, B. A.
In: Geophysical Research Letters, 36, 2009, 16
Medientyp: E-Article
Sprache: Englisch
veröffentlicht:
American Geophysical Union (AGU)
Schlagwörter:
author_facet Jones, G. H.
Arridge, C. S.
Coates, A. J.
Lewis, G. R.
Kanani, S.
Wellbrock, A.
Young, D. T.
Crary, F. J.
Tokar, R. L.
Wilson, R. J.
Hill, T. W.
Johnson, R. E.
Mitchell, D. G.
Schmidt, J.
Kempf, S.
Beckmann, U.
Russell, C. T.
Jia, Y. D.
Dougherty, M. K.
Waite, J. H.
Magee, B. A.
Jones, G. H.
Arridge, C. S.
Coates, A. J.
Lewis, G. R.
Kanani, S.
Wellbrock, A.
Young, D. T.
Crary, F. J.
Tokar, R. L.
Wilson, R. J.
Hill, T. W.
Johnson, R. E.
Mitchell, D. G.
Schmidt, J.
Kempf, S.
Beckmann, U.
Russell, C. T.
Jia, Y. D.
Dougherty, M. K.
Waite, J. H.
Magee, B. A.
author Jones, G. H.
Arridge, C. S.
Coates, A. J.
Lewis, G. R.
Kanani, S.
Wellbrock, A.
Young, D. T.
Crary, F. J.
Tokar, R. L.
Wilson, R. J.
Hill, T. W.
Johnson, R. E.
Mitchell, D. G.
Schmidt, J.
Kempf, S.
Beckmann, U.
Russell, C. T.
Jia, Y. D.
Dougherty, M. K.
Waite, J. H.
Magee, B. A.
spellingShingle Jones, G. H.
Arridge, C. S.
Coates, A. J.
Lewis, G. R.
Kanani, S.
Wellbrock, A.
Young, D. T.
Crary, F. J.
Tokar, R. L.
Wilson, R. J.
Hill, T. W.
Johnson, R. E.
Mitchell, D. G.
Schmidt, J.
Kempf, S.
Beckmann, U.
Russell, C. T.
Jia, Y. D.
Dougherty, M. K.
Waite, J. H.
Magee, B. A.
Geophysical Research Letters
Fine jet structure of electrically charged grains in Enceladus' plume
General Earth and Planetary Sciences
Geophysics
author_sort jones, g. h.
spelling Jones, G. H. Arridge, C. S. Coates, A. J. Lewis, G. R. Kanani, S. Wellbrock, A. Young, D. T. Crary, F. J. Tokar, R. L. Wilson, R. J. Hill, T. W. Johnson, R. E. Mitchell, D. G. Schmidt, J. Kempf, S. Beckmann, U. Russell, C. T. Jia, Y. D. Dougherty, M. K. Waite, J. H. Magee, B. A. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/2009gl038284 <jats:p>By traversing the plume erupting from high southern latitudes on Saturn's moon Enceladus, Cassini orbiter instruments can directly sample the material therein. Cassini Plasma Spectrometer, CAPS, data show that a major plume component comprises previously‐undetected particles of nanometer scales and larger that bridge the mass gap between previously observed gaseous species and solid icy grains. This population is electrically charged both negative and positive, indicating that subsurface triboelectric charging, i.e., contact electrification of condensed plume material may occur through mutual collisions within vents. The electric field of Saturn's magnetosphere controls the jets' morphologies, separating particles according to mass and charge. Fine‐scale structuring of these particles' spatial distribution correlates with discrete plume jets' sources, and reveals locations of other possible active regions. The observed plume population likely forms a major component of high velocity nanometer particle streams detected outside Saturn's magnetosphere.</jats:p> Fine jet structure of electrically charged grains in Enceladus' plume Geophysical Research Letters
doi_str_mv 10.1029/2009gl038284
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title Fine jet structure of electrically charged grains in Enceladus' plume
title_unstemmed Fine jet structure of electrically charged grains in Enceladus' plume
title_full Fine jet structure of electrically charged grains in Enceladus' plume
title_fullStr Fine jet structure of electrically charged grains in Enceladus' plume
title_full_unstemmed Fine jet structure of electrically charged grains in Enceladus' plume
title_short Fine jet structure of electrically charged grains in Enceladus' plume
title_sort fine jet structure of electrically charged grains in enceladus' plume
topic General Earth and Planetary Sciences
Geophysics
url http://dx.doi.org/10.1029/2009gl038284
publishDate 2009
physical
description <jats:p>By traversing the plume erupting from high southern latitudes on Saturn's moon Enceladus, Cassini orbiter instruments can directly sample the material therein. Cassini Plasma Spectrometer, CAPS, data show that a major plume component comprises previously‐undetected particles of nanometer scales and larger that bridge the mass gap between previously observed gaseous species and solid icy grains. This population is electrically charged both negative and positive, indicating that subsurface triboelectric charging, i.e., contact electrification of condensed plume material may occur through mutual collisions within vents. The electric field of Saturn's magnetosphere controls the jets' morphologies, separating particles according to mass and charge. Fine‐scale structuring of these particles' spatial distribution correlates with discrete plume jets' sources, and reveals locations of other possible active regions. The observed plume population likely forms a major component of high velocity nanometer particle streams detected outside Saturn's magnetosphere.</jats:p>
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author Jones, G. H., Arridge, C. S., Coates, A. J., Lewis, G. R., Kanani, S., Wellbrock, A., Young, D. T., Crary, F. J., Tokar, R. L., Wilson, R. J., Hill, T. W., Johnson, R. E., Mitchell, D. G., Schmidt, J., Kempf, S., Beckmann, U., Russell, C. T., Jia, Y. D., Dougherty, M. K., Waite, J. H., Magee, B. A.
author_facet Jones, G. H., Arridge, C. S., Coates, A. J., Lewis, G. R., Kanani, S., Wellbrock, A., Young, D. T., Crary, F. J., Tokar, R. L., Wilson, R. J., Hill, T. W., Johnson, R. E., Mitchell, D. G., Schmidt, J., Kempf, S., Beckmann, U., Russell, C. T., Jia, Y. D., Dougherty, M. K., Waite, J. H., Magee, B. A., Jones, G. H., Arridge, C. S., Coates, A. J., Lewis, G. R., Kanani, S., Wellbrock, A., Young, D. T., Crary, F. J., Tokar, R. L., Wilson, R. J., Hill, T. W., Johnson, R. E., Mitchell, D. G., Schmidt, J., Kempf, S., Beckmann, U., Russell, C. T., Jia, Y. D., Dougherty, M. K., Waite, J. H., Magee, B. A.
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description <jats:p>By traversing the plume erupting from high southern latitudes on Saturn's moon Enceladus, Cassini orbiter instruments can directly sample the material therein. Cassini Plasma Spectrometer, CAPS, data show that a major plume component comprises previously‐undetected particles of nanometer scales and larger that bridge the mass gap between previously observed gaseous species and solid icy grains. This population is electrically charged both negative and positive, indicating that subsurface triboelectric charging, i.e., contact electrification of condensed plume material may occur through mutual collisions within vents. The electric field of Saturn's magnetosphere controls the jets' morphologies, separating particles according to mass and charge. Fine‐scale structuring of these particles' spatial distribution correlates with discrete plume jets' sources, and reveals locations of other possible active regions. The observed plume population likely forms a major component of high velocity nanometer particle streams detected outside Saturn's magnetosphere.</jats:p>
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spelling Jones, G. H. Arridge, C. S. Coates, A. J. Lewis, G. R. Kanani, S. Wellbrock, A. Young, D. T. Crary, F. J. Tokar, R. L. Wilson, R. J. Hill, T. W. Johnson, R. E. Mitchell, D. G. Schmidt, J. Kempf, S. Beckmann, U. Russell, C. T. Jia, Y. D. Dougherty, M. K. Waite, J. H. Magee, B. A. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/2009gl038284 <jats:p>By traversing the plume erupting from high southern latitudes on Saturn's moon Enceladus, Cassini orbiter instruments can directly sample the material therein. Cassini Plasma Spectrometer, CAPS, data show that a major plume component comprises previously‐undetected particles of nanometer scales and larger that bridge the mass gap between previously observed gaseous species and solid icy grains. This population is electrically charged both negative and positive, indicating that subsurface triboelectric charging, i.e., contact electrification of condensed plume material may occur through mutual collisions within vents. The electric field of Saturn's magnetosphere controls the jets' morphologies, separating particles according to mass and charge. Fine‐scale structuring of these particles' spatial distribution correlates with discrete plume jets' sources, and reveals locations of other possible active regions. The observed plume population likely forms a major component of high velocity nanometer particle streams detected outside Saturn's magnetosphere.</jats:p> Fine jet structure of electrically charged grains in Enceladus' plume Geophysical Research Letters
spellingShingle Jones, G. H., Arridge, C. S., Coates, A. J., Lewis, G. R., Kanani, S., Wellbrock, A., Young, D. T., Crary, F. J., Tokar, R. L., Wilson, R. J., Hill, T. W., Johnson, R. E., Mitchell, D. G., Schmidt, J., Kempf, S., Beckmann, U., Russell, C. T., Jia, Y. D., Dougherty, M. K., Waite, J. H., Magee, B. A., Geophysical Research Letters, Fine jet structure of electrically charged grains in Enceladus' plume, General Earth and Planetary Sciences, Geophysics
title Fine jet structure of electrically charged grains in Enceladus' plume
title_full Fine jet structure of electrically charged grains in Enceladus' plume
title_fullStr Fine jet structure of electrically charged grains in Enceladus' plume
title_full_unstemmed Fine jet structure of electrically charged grains in Enceladus' plume
title_short Fine jet structure of electrically charged grains in Enceladus' plume
title_sort fine jet structure of electrically charged grains in enceladus' plume
title_unstemmed Fine jet structure of electrically charged grains in Enceladus' plume
topic General Earth and Planetary Sciences, Geophysics
url http://dx.doi.org/10.1029/2009gl038284