Electron, Proton, and Alpha Monitor on the Advanced Composition Explorer spacecraft
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The Electron, Proton, and Alpha Monitor (EPAM) is designed to make measurements of ions and electrons over a broad range of energy and intensity. Through five separate solid-state detector telescopes oriented so as to provide nearly full coverage of the unit-sphere, EPAM can uniquely distinguish ions (Ei≳50 keV) and electrons (Ee≳40 keV) providing the context for the measurements of the high sensitivity instruments on ACE. Using a ΔE×E telescope, the instrument can determine ion elemental abundances (E≳0.5 MeV nucl−1). The large angular coverage and high time resolution will serve to alert the other instruments on ACE of interesting anisotropic events. The experiment is controlled by a microprocessor-based data system, and the entire instrument has been reconfigured from the HI-SCALE instrument on the Ulysses spacecraft. Inflight calibration is achieved using a variety of radioactive sources mounted on the reclosable telescope covers. Besides the coarse (8 channel) ion and (4 channel) electron energy spectra, the instrument is also capable of providing energy spectra with 32 logarithmically spaced channels using a pulse-height-analyzer. The instrument, along with its mounting bracket and radiators weighs 11.8 kg and uses about 4.0 W of power. To demonstrate some of the capabilities of the instrument, some initial performance data are included from a solar energetic particle event in November 1997.
KeywordsSolar Energetic Particle Event Energy Channel Rate Channel Ulysses Spacecraft Large Solar Energetic Particle Event
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- Chiu, M. C., von-Mehlem, U. I., Willey, C. E., Betenbaugh, T. M., Maynard, J. J., Krein, J. A., Conde, R. F., Gray, W. T., Hunt, Jr., J. W., Mosher, L. E., McCullough, M. G., Panneton, P. E., Staiger, J. P., and Rodberg, E. H.: 1998, ‘ACE, Spacecraft’, Space Sci. Rev. 86, 257.CrossRefADSGoogle Scholar
- Lanzerotti, L. J., Armstrong, T. P., Maclennan, C. G., Simnett, G. M., Cheng, A. F., Gold, R. E., Thomson, D. J., Krimigis, S. M., Anderson, K. A., Hawkins, S. E., III, Pick, M., Roelof, E. C., Sarris, E. T., and Tappin, S. J.: 1993, ‘Measurements of Hot Plasma in the Magnetosphere of Jupiter’, Planetary Space Sci. 41, 893.CrossRefADSGoogle Scholar
- Lanzerotti, L. J., Gold, R. E., Anderson, K. A., Armstrong, T. P., Lin, R. P., Krimigis, S. M., Pick, M., Roelof, E. C., Sarris, E. T., Simnett, G., and Frain, W. E.: 1983, in K.-P. Wenzel, R. G. Marsden, and B. Battrick (eds.), ‘The ISPM Experiment for Spectra, Composition, and Anisotropy Measurements of Charged Particles at Low Energies’, The International Solar Polar Mission — Its Scientific Investigations, Noordwijk, The Netherlands, 141–154.Google Scholar
- Lanzerotti, L. J., Gold, R. E., Anderson, K. A., Armstrong, T. P., Lin, R. P., Krimigis, S. M., Pick, M., Roelof, E. C., Sarris, E. T., Simnett, G., and Frain, W. E.: 1992, ‘Heliosphere Instrument for Spectra, Composition, and Anisotropy at Low Energies’, Astron. Astrophys. 92, 349.ADSGoogle Scholar