Physics – Optics
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1744...13r&link_type=abstract
Proc. SPIE Vol. 1744, p. 13-18, Instrumentation for Magnetospheric Imagery, Supriya Chakrabarti; Ed.
Physics
Optics
Scientific paper
Simulated images of extreme ultraviolet (EUV) emissions form energetic outflowing 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 plasmaspheric 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 outflowing 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.
Catura Richard C.
Chiu Yam T.
Collin Henry L.
Garrido Dante E.
Robinson Bob M.
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