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Publications for 1992
- Electrostatic Waves Due to Field-Aligned Electron Beams in the Low Latitude Boundary Layer, V. Peroomian, et. al
- The Polar Cap Environment of Outflowing O, J.L. Horwitz, et. al
- Funnel Shaped Low Frequency Equatorial Waves, S.A. Boardsen, et. al
- O and He Restricted and Extended (Bi-Modal) Ion Conic Distributions, W.K. Peterson, et. al
- Coordinated Measurements from the CRRES, DE-1, and DMSP Satellites on Feburary 18, 1991, W.K. Peterson
- Interplanetary Magnetic Flux: Measurement and Balance, D. J. McComas, et. al
- The Observations of a New Class of Upstream Waves with Periods Near 3 Seconds, J. T. Gosling
- Coronal Mass Ejections: The Link Between Solar and Geomagnetic Activity, (extended abstract), Eruptive Solar Flares, J. T. Gosling, et. al
- Magnetic Topology of Coronal Mass Ejections Based on ISEE-3 Observations of Bidirectional Electron Fluxes at 1 AU, J. L Phillips, et. al
- Regulation of the Interplanetary Magnetic Field, D. J. McComas, et. al
- Counterstreaming Solar Wind Halo Electron Events on Open Field Lines?, J. T. Gosling, et. al
- Quantitative Analysis of Bidirectional Electron Fluxes Within Coronal Mass Ejections at 1 AU, J. L. Phillips, et. al
- Counterstreaming Solar Wind Halo Electron Events: Solar Cycle Variations, J. T. Gosling, et. al
- In Situ Observations of Coronal Mass Ejections in Interplanetary Space, Eruptive Solar Flares, J. T. Gosling
- Solar Wind Thermal Distributions, J. L. Phillips, et. al
- The Ulysses Solar Wind Plasma Investigation: Description and Initial In-Ecliptic Results, S. J. Bame, et. al
- Solar Wind Halo Electrons from 1 - 4 AU, D. J. McComas, et. al
- Ulysses Plasma Observations of Coronal Mass Ejections Near 2.5 AU, J. L. Phillips, et. al
- ISEE-1 and ISEE-2 Observations of the High Beta Shock, M. H. Farris, et. al
- Low Energy Neutral Atom Imaging, Instrumentation for Magnetospheric Imagery, D. J. McComas, et. al
- Jupiter's Magnetosphere: Plasma Description from the Ulysses Flyby, S. J. Bame, et. al
Last Updated:
Mon, 20 May 13 09:48:27 -0600
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