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Ulysses HISCALE Data Analysis Handbook

 

Appendix 9  Geometric Factor Study for the Deflected and Unscattered Electrons of HISCALE (Buckley MS Thesis)

 

The specific aspect that this investigation focuses on are the electrons that enter LEMS30.  The instrument has been designed such that these electrons are deflected into the back of the CA, as shown in Figure A9-2.  The detector is able to differentiate four energy ranges of electrons, which are denoted as energy passbands DE1-DE4.  Since it is impossible for the more massive ions to experience such a deflection, the count rates for these channels are purely electrons.  It is the goal of this study to determine the geometric factor for these deflected electrons for the four energy channels.

 

Figure A9-2  Electrons entering the LEMS30 aperture are deflected into the back of the Composition Aperture.

 

Figure A9.2

 

 

Next: Chapter 2 - The Geometric Factor and Fluxes

 

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Updated 8/8/19, Cameron Crane

QUICK FACTS

Manufacturer: ESA provided the Ulysses spacecraft, NASA provided the power supply, and various others provided its instruments.

Mission End Date: June 30, 2009

Destination: The inner heliosphere of the sun away from the ecliptic plane

Orbit:  Elliptical orbit transversing the polar regions of the sun outside of the ecliptic plane