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The RHESSI Imaging Concept

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The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI)

Abstract

The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) observes solar hard X-rays and gamma-rays from 3 keV to 17 MeV with spatial resolution as high as 2.3 arc sec. Instead of focusing optics, imaging is based on nine rotating modulation collimators that time-modulate the incident flux as the spacecraft rotates. Starting from the arrival time of individual photons, ground-based software then uses the modulated signals to reconstruct images of the source. The purpose of this paper is to convey both an intuitive feel and the mathematical basis for this imaging process. Following a review of the relevant hardware, the imaging principles and the basic back-projection method are described, along with their relation to Fourier transforms. Several specific algorithms (Clean, MEM, Pixons and Forward-Fitting) applicable to RHESSI imaging are briefly described. The characteristic strengths and weaknesses of this type of imaging are summarized.

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Author information

Authors and Affiliations

  1. Space Sciences Laboratory, University of California, Berkeley, CA, 94720, USA

    G. J. Hurford, A. Csillaghy, S. Krucker, R. P. Lin, J. Mctiernan & D. M. Smith

  2. Astronomy Department, University of Maryland, College Park, MD, 20742, USA

    E. J. Schmahl

  3. Lab for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA

    E. J. Schmahl, R. A. Schwartz & B. R. Dennis

  4. NASA Goddard Space Flight Center / SSAI, Greenbelt, MD, 20771, USA

    R. A. Schwartz

  5. Department of Physics and Astronomy, The Open University, Milton Keynes, MK7 6AA, UK

    A. J. Conway

  6. Solar & Astrophysics Laboratory, Dept. L9-41, Lockheed Martin Advanced Technology Center, Palo Alto, CA, 94304, USA

    M. J. Aschwanden & T. R. Metcalf

  7. University of Applied Sciences, CH-5210, Windisch, Switzerland

    A. Csillaghy

  8. Department of Physics and Astronomy, Rice University, Houston, TX, 77005, USA

    C. Johns-Krull

  9. Department of Physics, University of California, Berkeley, CA, 94720, USA

    R. P. Lin

  10. Department of Physics, Montana State University, Bozeman, MT, 59717, USA

    J. Sato

Authors
  1. G. J. Hurford
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  2. E. J. Schmahl
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  3. R. A. Schwartz
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  4. A. J. Conway
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  5. M. J. Aschwanden
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  6. A. Csillaghy
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  7. B. R. Dennis
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  8. C. Johns-Krull
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  9. S. Krucker
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  10. R. P. Lin
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  11. J. Mctiernan
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  12. T. R. Metcalf
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  13. J. Sato
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  14. D. M. Smith
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Editor information

Editors and Affiliations

  1. Space Sciences Laboratory and Physics Department, University of California, Berkeley, USA

    Robert P. Lin

  2. Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, USA

    Brian R. Dennis

  3. Institute of Astronomy, ETH-Zentrum, Zürich, Switzerland

    Arnold O. Benz

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© 2003 Springer Science+Business Media Dordrecht

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Hurford, G.J. et al. (2003). The RHESSI Imaging Concept. In: Lin, R.P., Dennis, B.R., Benz, A.O. (eds) The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI). Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3452-3_3

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  • DOI: https://doi.org/10.1007/978-94-017-3452-3_3

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-6212-3

  • Online ISBN: 978-94-017-3452-3

  • eBook Packages: Springer Book Archive

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