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Proceedings Paper

Instrumental and observational requirements for space-based imaging of magnetospheric emissions
Author(s): Bob M. Robinson; Yam T. Chiu; Richard C. Catura; Henry L. Collin; Dante Espino Garrido; Roger W. Smith
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Paper Abstract

Simulated images of extreme ultraviolet (EUV) emissions from energetic outfiowing ions have been constructed to study techniques for remotely sensing the dynamic behavior of hot plasmas in the near-Earth environment. These calculations include realistic assumptions about the energetic ion outflow from high latitudes and take into account the effects of cold plasmasphenc and ionospheric ions. The energetic ion outflow is determined from a statistical study based on five years of measurements from the Energetic Ion Composition Spectrometer on Dynamics Explorer 1. The simulated images change significantly with viewing geometry and certain spacecraft locations are clearly favorable for observing emissions from energetic ions. For example, for a near equatorial orbit, viewing locations greater than 9 Earth radii are required to observe outfiowing ions above the cold plasmaspheric background. We will discuss other important considerations for magnetospheric imaging including the sensitivity requirements of the detector. In particular, we consider the performance of multi-layer optics for EUV wavelengths.

Paper Details

Date Published: 1 June 1992
PDF: 6 pages
Proc. SPIE 1744, Instrumentation for Magnetospheric Imagery, (1 June 1992); doi: 10.1117/12.60575
Show Author Affiliations
Bob M. Robinson, Lockheed Palo Alto Research Lab. (United States)
Yam T. Chiu, Lockheed Palo Alto Research Lab. (United States)
Richard C. Catura, Lockheed Palo Alto Research Lab. (United States)
Henry L. Collin, Lockheed Palo Alto Research Lab. (United States)
Dante Espino Garrido, Univ. of Alaska/Fairbanks (United States)
Roger W. Smith, Univ. of Alaska/Fairbanks (United States)


Published in SPIE Proceedings Vol. 1744:
Instrumentation for Magnetospheric Imagery
Supriya Chakrabarti, Editor(s)

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