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1

Summer Study Program in Geophysical Fluid Dynamics (1988 Woods Hole Oceanographic Institution). Order and disorder in planetary dynamos. Woods Hole Oceanographic Institution, 1988.

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2

Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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3

Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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4

Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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5

Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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6

Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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7

Evans, D. R. Non-dipolar magnetic field models and patterns of radio emission: Uranus and Neptune compared : final report. National Aeronautics and Space Administration, 1994.

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8

United States. National Aeronautics and Space Administration., ed. Non-dipolar magnetic field models and patterns of radio emission: Uranus and Neptune compared : final report. National Aeronautics and Space Administration, 1994.

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9

United States. National Aeronautics and Space Administration., ed. Non-dipolar magnetic field models and patterns of radio emission: Uranus and Neptune compared : final report. National Aeronautics and Space Administration, 1994.

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10

L, Kaufmann Richard, and United States. National Aeronautics and Space Administration., eds. Force balance and substorm effects in the magnetotail. National Aeronautics and Space Administration, 1997.

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11

Karousatos, Tassos A. The planet sun. Laboratory of Magneto-Optical Research, 1985.

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12

L, Green James, and United States. National Aeronautics and Space Administration., eds. Modeling and inestigative stuides of Jovian low frequency emissions: Final report. National Aeronautics and Space Administration, 1986.

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13

United States. National Aeronautics and Space Administration., ed. Solar wind effects on atmospheres of the weakly magnetized bodies--Mars, Titan, and the moon: Final technical report. National Aeronautics and Space Administration, 1996.

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14

Luhmann, Janet G. Solar wind effects on atmospheres of the weakly magnetized bodies--Mars, Titan, and the moon: Final technical report. National Aeronautics and Space Administration, 1996.

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15

Malkus, Willem V. R. Order and disorder in planetary dynamos: Summer study program in geophysical fluid dynamics. Woods Hole Oceanographic Institution, 1988.

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16

United States. National Aeronautics and Space Administration., ed. "Studies of plasma flow past Jupiters satellite Io": Progress report: second year (2/07/96-2/06/97) : NASA contract: NASW-4941. Science Applications International Corporation, 1997.

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17

United States. National Aeronautics and Space Administration., ed. Global auroral imaging for the Dynamics Explorer mission: NAG5-483 : summary of research, November 01, 1984-January 31, 1998. Dept. of Physics and Astronomy, University of Iowa, 1998.

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18

United States. National Aeronautics and Space Administration., ed. Global auroral imaging for the Dynamics Explorer mission: NAG5-483 : summary of research, November 01, 1984-January 31, 1998. Dept. of Physics and Astronomy, University of Iowa, 1998.

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19

United States. National Aeronautics and Space Administration., ed. MHD modeling of the interaction of the solar wind with Venus: Final report, NASA grant no. NAGW-3779, SwRI project no. 15-6083. Southwest Research Institute, Venus Data Analysis Program, 1996.

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20

United States. National Aeronautics and Space Administration., ed. MHD modeling of the interaction of the solar wind with Venus: Final report, NASA grant no. NAGW-3779, SwRI project no. 15-6083. Southwest Research Institute, Venus Data Analysis Program, 1996.

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21

United States. National Aeronautics and Space Administration., ed. Analysis of magnetic field data from the Pioneer Venus orbiter: Final technical report for NASA grant NAG 2-501. National Aeronautics and Space Administration, 1994.

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22

United States. National Aeronautics and Space Administration., ed. Studies of plasma flow past Jupiter's satellite Io: Progress report, first year [2/07/95 - 2/06/96). National Aeronautics and Space Administration, 1996.

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23

United States. National Aeronautics and Space Administration., ed. Final report on Venus data analysis program grant number NAGW-3497, "Plasma waves in the magnetosheath of Venus". National Aeronautics and Space Administration, 1996.

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24

Rainer, Bauske, and United States. National Aeronautics and Space Administration., eds. The Shoemaker-Levy 9/Jupiter impact: Auroral and high energy processes : final report for NASA grant NAGW-4797; original funding period: September 1, 1995 to August 31, 1996, extended at no additional cost to September 30, 1997. National Aeronautics and Space Administration, 1997.

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25

Rainer, Bauske, and United States. National Aeronautics and Space Administration., eds. The Shoemaker-Levy 9/Jupiter impact: Auroral and high energy processes : final report for NASA grant NAGW-4797; original funding period: September 1, 1995 to August 31, 1996, extended at no additional cost to September 30, 1997. National Aeronautics and Space Administration, 1997.

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26

Jones, Douglas E. Pioneer 10 and 11 (Jupiter and Saturn) magnetic field experiments. National Aeronautics and Space Administration, 1986.

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27

Sterenborg, Michael Glenn. Topical Study of Planetary Magnetic Fields. 2011.

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28

Balogh, A., K. H. Glaßmeier, U. R. Christensen, and D. Breuer. Planetary Magnetism. Springer, 2012.

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29

Boundary value problem for the solution of magnetic cutoff rigidities and some special applications. National Aeronautics and Space Administration, Jet Propulsion Laboratory, California Institute of Technology, 1987.

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30

Studies of plasma flow past Jupiter's satellite Io: Progress report, first year [2/07/95 - 2/06/96). National Aeronautics and Space Administration, 1996.

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31

The Shoemaker-Levy 9/Jupiter impact: Auroral and high energy processes : final report for NASA grant NAGW-4797; original funding period: September 1, 1995 to August 31, 1996, extended at no additional cost to September 30, 1997. National Aeronautics and Space Administration, 1997.

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32

The Shoemaker-Levy 9/Jupiter impact: Auroral and high energy processes : final report for NASA grant NAGW-4797; original funding period: September 1, 1995 to August 31, 1996, extended at no additional cost to September 30, 1997. National Aeronautics and Space Administration, 1997.

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33

Eland, John, and Raimund Feifel. Double Photoionisation Spectra of Molecules. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198788980.001.0001.

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This book contains spectra of the doubly charged positive ions (dications) of some 75 molecules, including the major constituents of terrestrial and planetary atmospheres and prototypes of major chemical groups. It is intended to be a new resource for research in all areas of molecular spectroscopy involving high energy environments, both terrestrial and extra-terrestrial. All the spectra have been produced by photoionisation using laboratory lamps or synchrotron radiation and have been measured using the magnetic bottle time-of-flight technique by coincidence detection of correlated electron
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34

Kennel, Charles F. Convection and Substorms. Oxford University Press, 1996. http://dx.doi.org/10.1093/oso/9780195085297.001.0001.

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The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region. Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection
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