Instrument Information |
|
IDENTIFIER | urn:esa:psa:context:instrument:uly.hiscale::1.0 |
NAME |
HELIOSPHERIC INST-SPECTRA,COMPOSITION,ANISOTROPY AT LOW ENER |
TYPE |
PARTICLE DETECTOR |
DESCRIPTION |
Instrument Overview =================== (excerpted from: [LANZEROTTIETAL1992]) Abstract. -- The Heliosphere Instrument for Spectra, Composition, and Anisotropy at Low Energies (HI-SCALE) is designed to make measurements of interplanetary ions and electrons throughout the entire Ulysses mission. The ions (Ei >50 keV) and electrons (Ee >30 keV) are identified uniquely and detected by five separate solid-state detector telescopes that are oriented to give nearly complete pitch-angle coverage (i.e., coverage of essentially 4 [pi] ster) from the spinning spacecraft. Ion elemental abundances are determined by a delta E vs E telescope using a thin (5 [micrometer]) front solid state detector element in a three-element telescope. Experiment operation is controlled by a microprocessor-based data system. Inflight calibration is provided by radioactive sources mounted on telescope covers which can be closed for calibration purposes and for radiation protection during the course of the mission. Ion and electron spectral information is determined using both broad-energy-range rate channels and a 32 channel pulse-height analyser (channels spaced logarithmically) for more detailed spectra. The instrument weighs 5.775 kg and uses 4.0 W of power. Some initial in-ecliptic measurements are presented which demonstrate the features of the instrument. References ---------- HISCALE References (cited in [ARMSTRONG&SAHI1996]) Curtis, D.W., ISPM/Ulysses LAN Data Processing Software Status, Dec. 1986. Gold R.E., LAN Accelerator Calibration Test Plan, August 1991. Guynn D.R. Jr., LAN Experiment Data System Performance and Interface Specification, June 1992. Kohl, J.W., J.H. Crawford, Calibration of Solar Polar Energy Model LAN-2B Detector Head at GSFC Low Energy Accelerator, July 1986. Simnett, G.M., R.E. Gold, The RTG Background in the LAN Experiment and the Shielding Required to Control It, April 1980. Tappin, S.J., HSIO-HiScale I/O Library, June 1991. Ximenez de Ferran S., Ulysses Spin Reference Pulse, May 1985. |
MODEL IDENTIFIER | |
NAIF INSTRUMENT IDENTIFIER |
not applicable |
SERIAL NUMBER |
not applicable |
REFERENCES |
Armstrong, T.P., and R. Sahi, Ulysses HISCALE Data Analysis Handbook, Dept.
of Physics and Astronomy, Univ. of Kansas, Lawrence, KS, 66045, April
1996. Armstrong, T.P., Passbands & Efficiencies for LEMS, LEFS and WART Channels, University of Kansas, May 1992. Lanzerotti, L.J., R.E. Gold, K.A. Anderson, T.P. Armstrong, R.P. Lin, S.M. Krimigis, M. Pick, E.C. Roelof, E.T. Sarris, G.M. Simnett, and W.E. Frain, Heliosphere instrument for spectra, composition and anisotropy at low energies, Astron. Astrophys. Suppl. Ser. 92, 349-363, 1992. Maclennan C.G., and Armstrong T.P., LAN Cover-Close Calibrations, AT&T Bell Laboratories, May 1995. Maclennan, C.G., User's Guide to LAN 360, AT&T Bell Laboratories, Aug. 1992. Tappin, S.J., HISCALE IDL display System (IDL-HS), University of Birmingham, June 1992. Townsend, J.P. Jr., Ulysses Pulse Height Analysis documentation, JHU, Applied Physics Laboratory, July 1990. |