Search Results - "McDonnell, J A"

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  1. 1

    Dust Measurements in the Coma of Comet 81P/Wild 2 by the Dust Flux Monitor Instrument by Tuzzolino, Anthony J., Economou, Thanasis E., Clark, Ben C., Tsou, Peter, Brownlee, Donald E., Green, Simon F., McDonnell, J. A. M., McBride, Neil, Melusine T. S. H. Colwell

    “…We present measurements of the dust particle flux and mass distribution from the Stardust Dust Flux Monitor Instrument (DFMI) throughout the flyby of comet…”
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    Journal Article
  2. 2

    The composition of Saturn's E ring by Hillier, Jon K., Green, S. F., McBride, N., Schwanethal, J. P., Postberg, F., Srama, R., Kempf, S., Moragas-Klostermeyer, G., McDonnell, J. A. M., Grün, E.

    “…We present the first in situ direct measurement of the composition of particles in Saturn's rings. The Cassini cosmic dust analyser (CDA) measured the mass…”
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    Journal Article
  3. 3

    A water quality monitoring network design methodology for the selection of critical sampling points: Part I by STROBL, R. O, ROBILLARD, P. D, SHANNON, R. D, DAY, R. L, MCDONNELL, A. J

    “…The principal instrument to temporally and spatially manage water resources is a water quality monitoring network. However, to date in most cases, there is a…”
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  4. 4

    The Open University planetary impact facility: A compact two-stage light gas gun for all impact angles by McDonnell, J.A.M.

    “…For liquid and planetary regolith target studies, requiring a horizontal target plain, a two-stage light gas gun (LGG) was designed by UniSpaceKent and…”
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    Journal Article Conference Proceeding
  5. 5

    water quality monitoring network design methodology for the selection of critical sampling points: Part II by Strobl, R. O, Robillard, P. D, Day, R. L, Shannon, R. D, McDonnell, A. J

    Published in Environmental monitoring and assessment (01-11-2006)
    “…In order to resolve the spatial component of the design of a water quality monitoring network, a methodology has been developed to identify the critical…”
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  6. 6

    The dust mass distribution of comet 81P/Wild 2 by Green, S. F., McDonnell, J. A. M., McBride, N., Colwell, M. T. S. H., Tuzzolino, A. J., Economou, T. E., Tsou, P., Clark, B. C., Brownlee, D. E.

    Published in Journal of Geophysical Research - Planets (01-12-2004)
    “…The Dust Flux Monitor Instrument (DFMI) made direct measurements of the dust environment in the mass range 10−14 < m < 10−5 kg at comet 81P/Wild 2 during the…”
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    Discovery of Jovian dust streams and interstellar grains by the Ulysses spacecraft by Gruen, E., Zook, H. A., Baguhl, M., Balogh, A., Bame, S. J., Fechtig, H., Forsyth, R., Hanner, M. S., Horanyi, M., Kissel, J.

    Published in Nature (London) (01-04-1993)
    “…Within 1 AU from Jupiter, the dust detector aboard the Ulysses spacecraft during the flyby on February 8, 1992 recorded periodic bursts of submicron dust…”
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    Galileo observes electromagnetically coupled dust in the Jovian magnetosphere by Grün, E., Krüger, H., Graps, A. L., Hamilton, D. P., Heck, A., Linkert, G., Zook, H. A., Dermott, S., Fechtig, H., Gustafson, B. A., Hanner, M. S., Horányi, M., Kissel, J., Lindblad, B. A., Linkert, D., Mann, I., McDonnell, J. A. M., Morfill, G. E., Polanskey, C., Schwehm, G., Srama, R.

    Published in Journal of Geophysical Research: Planets (30-08-1998)
    “…Measurements of dust coupled to the Jovian magnetosphere have been obtained with the dust detector on board the Galileo spacecraft. We report on data obtained…”
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    Journal Article Conference Proceeding
  11. 11

    Dust Measurements at High Ecliptic Latitudes by Baguhl, M., Hamilton, D. P., Grün, E., Dermott, S. F., Fechtig, H., Hanner, M. S., Kissel, J., B.-A. Lindblad, Linkert, D., Linkert, G., Mann, I., McDonnell, J. A. M., Morfill, G. E., Polanskey, C., Riemann, R., Schwehm, G., Staubach, P., Zook, H. A.

    “…Along Ulysses' path from Jupiter to the south ecliptic pole, the onboard dust detector measured a dust impact rate that varied slowly from 0.2 to 0.5 impacts…”
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    Dust Measurements During Galileo's Approach to Jupiter and Io Encounter by Grun, E, Hamilton, D.P, Riemann, R, Dermott, S, Fechtig, H, Gustafson, B.A, Hanner, M.S, Heck, A, Horanyi, M, Kissel, J, Kruger, H, Lindblad, B.A, Linkert, D, Linkert, G, Mann, I, McDonnell, J.A.M, Morfill, G.E, Polanskey, C, Schwehm, G, Srama, R, Zook, H.A

    “…About a hundred dust impacts per day were detected during the first week in December 1995 by Galileo during its approach to Jupiter. These impacts were caused…”
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  14. 14

    Stardust: Comet and interstellar dust sample return mission by Brownlee, D. E., Tsou, P., Anderson, J. D., Hanner, M. S., Newburn, R. L., Sekanina, Z., Clark, B. C., Hörz, F., Zolensky, M. E., Kissel, J., McDonnell, J. A. M., Sandford, S. A., Tuzzolino, A. J.

    Published in Journal of Geophysical Research - Planets (01-10-2003)
    “…Stardust, the 4th Discovery mission launched in February 1999, will collect coma samples from the recently deflected comet 81P/Wild 2 on 2 January 2004 and…”
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  15. 15

    Constraints from Galileo observations on the origin of jovian dust streams by Grün, E, Baguhl, M, Hamilton, D. P, Riemann, R, Zook, H. A, Dermott, S, Fechtig, H, Gustafson, B. A, Hanner, M. S, Horányi, M, Khurana, K. K, Kissel, J, Kivelson, M, Lindblad, B. A, Linkert, D, Linkert, G, Mann, I, McDonnell, J. A. M, Morfill, G. E, Polanskey, C, Schwehm, G, Srama, R

    Published in Nature (London) (30-05-1996)
    “…The Ulysses spacecraft detected streams of sub-micrometre-sized dust particles as it approached Jupiter in 1992. The directions from which the dust grains…”
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  16. 16

    Dust particle impacts during the Giotto encounter with comet Grigg-Skjellerup by McDonnell, J. A. M, McBride, N, Beard, R, Bussoletti, E, Colangeli, L, Eberhardt, P, Firth, J. G, Grard, R, Green, S. F, Greenberg, J. M, Grün, E, Hughes, D. W, Keller, H. U, Kissel, J, Lindblad, B. A, Mandeville, J.-C, Perry, C. H, Rembor, K, Rickman, H, Schwehm, G. H, Turner, R. F, Wallis, M. K, Zarnecki, J. C

    Published in Nature (London) (22-04-1993)
    “…Particle masses found during the Giotto spacecraft's encounter with the comet Grigg-Skjellerup suggest that the mass distribution of the cometary dust was…”
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    Composition of comet Halley dust particles from Giotto observations by Kissel, J., Buechler, K., Fechtig, H., Gruen, E., Jessberger, E. K., Brownlee, D. E., Clark, B. C., Hornung, K., Igenbergs, E. B., Sekanina, Z.

    Published in Nature (London) (15-05-1986)
    “…Mass spectra of cometary dust particles measured by the PIA dust particle analyzer aboard the Giotto spacecraft show some unexpected and striking features…”
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  18. 18

    Dust density and mass distribution near comet Halley from Giotto observations by Mcdonnell, J. A. M., Alexander, W. M., Burton, W. M., Bussoletti, E., Clark, D. H., Grard, J. L., Gruen, E., Hanner, M. S., Sekanina, Z., Hughes, D. W.

    Published in Nature (London) (15-05-1986)
    “…The density and the mass spectrum of the dust near comet Halley have been measured by the Giotto space probe's dust impact detection system. The dust spectrum…”
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  19. 19

    Stardust encounters comet 81P/Wild 2 by Tsou, P., Brownlee, D. E., Anderson, J. D., Bhaskaran, S., Cheuvront, A. R., Clark, B. C., Duxbury, T., Economou, T., Green, S. F., Hanner, M. S., Hörz, F., Kissel, J., McDonnell, J. A. M., Newburn, R. L., Ryan, R. E., Sandford, S. A., Sekanina, Z., Tuzzolino, A. J., Vellinga, J. M., Zolensky, M. E.

    Published in Journal of Geophysical Research - Planets (01-12-2004)
    “…Stardust successfully encountered comet 81P/Wild 2 on 2 January 2004 at a distance of 236.4 ± 1 km. All encounter investigations acquired valuable new and…”
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  20. 20

    Dust Flux Monitor Instrument for the Stardust mission to comet Wild 2 by Tuzzolino, A. J., Economou, T. E., McKibben, R. B., Simpson, J. A., McDonnell, J. A. M., Burchell, M. J., Vaughan, B. A. M., Tsou, P., Hanner, M. S., Clark, B. C., Brownlee, D. E.

    Published in Journal of Geophysical Research - Planets (01-10-2003)
    “…The Dust Flux Monitor Instrument (DFMI) is part of the Stardust instrument payload. The prime goal of the DFMI is to measure the particle flux, intensity…”
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