Ulysses HISCALE Data Analysis Handbook
Appendix 9 Geometric Factor Study for the Deflected and Unscattered Electrons of HISCALE (Buckley MS Thesis)
A9.3 Chapter 3 - The Specific Problem
The objective is to find the energy-dependent geometric factor for the deflected electrons of HISCALE. The method of approach is identical to that of Shodhan3, and much of the software needed to implement the following steps is adopted from her work. Basically, there are four main tasks one must accomplish.
1. Model the geometry of the detector and telescope system, picking an appropriate coordinate system.
2. Model the magnetic field created by the deflecting magnets.
3. Determine the solid angle of electron trajectories that escape the sensor system for a specified area on the detector, and sum over all these areas to obtain G.
4. Repeat steps 1-3 for different electron energies.
Step 1. Modeling the Detector and Telescope
Shodhan's method works on the assumption that the entire subsystem is modeled with plane polygons. To model the detector and telescope for the deflected electrons, the first step was to obtain the mechanical drawings of the HISCALE instrument, an example of which is shown in Figure A9-5. Next, a suitable origin must be chosen. Since Shodhan's software is used, it is important to adopt her coordinate system and a similar origin. The resulting coordinate system shown with respect to the rest of the HISCALE instrument is shown in Figure A9-6, and the resulting model for the geometry is shown in Figures A9-7a, b, c.
A listing of the coordinate labels, as well as plane coefficients needed in the software, is given in Section A9.5.
Return to HISCALE List of Appendices
Return to Ulysses HISCALE Data Analysis Handbook Table of Contents
Updated 8/8/19, Cameron Crane
QUICK FACTS
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