P
Paul D. Craven
Researcher at Marshall Space Flight Center
Publications - 74
Citations - 1965
Paul D. Craven is an academic researcher from Marshall Space Flight Center. The author has contributed to research in topics: Magnetosphere & Polar wind. The author has an hindex of 21, co-authored 74 publications receiving 1832 citations.
Papers
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Global Core Plasma Model
TL;DR: The Global Core Plasma Model (GCPM) as discussed by the authors is an attempt to assimilate previous empirical evidence and regional models into a continuous, smooth model of thermal plasma density in the inner magnetosphere.
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Ionospheric mass ejection in response to a CME
Thomas E. Moore,W. K. Peterson,Christopher T. Russell,Michael O. Chandler,Michael R. Collier,H. L. Collin,Paul D. Craven,R. J. Fitzenreiter,Barbara L. Giles,C. J. Pollock +9 more
TL;DR: This paper reported a direct ionospheric plasma outflow response to the incidence of an interplanetary shock and associated coronal mass ejection (CME) upon the earth's magnetosphere.
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Polar wind survey with the Thermal Ion Dynamics Experiment/Plasma Source Instrument suite aboard POLAR
Yi-Jiun Su,J. L. Horwitz,T. E. Moore,Barbara L. Giles,Michael O. Chandler,Paul D. Craven,Masafumi Hirahara,C. J. Pollock +7 more
TL;DR: The results of a survey of the polar wind characteristics for H +, He +, and O + as observed by TIDE at ∼5000 km and ∼8 R E altitudes over the polar cap during April-May 1996 were presented in this paper.
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An empirical model of the earth's plasmasphere
TL;DR: In this paper, an empirical model for plasmaspheric low-energy plasma consisting of H(+) was developed from a data base derived from measurements taken by the Retarding Ion Mass Spectrometer on the DE-1 satellite.
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Relative concentration of He+ in the inner magnetosphere as observed by the DE 1 retarding ion mass spectrometer
TL;DR: In this article, the He(+) to H(+) density ratios as a function of altitude, latitude, season, local time, geomagnetic and solar activity were examined using the retarding ion mass spectrometer on the Dynamics Explorer I.