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

Mission Description and Early Results

  • Robert P. Lin
  • Brian R. Dennis
  • Arnold O. Benz

Table of contents

  1. Front Matter
    Pages i-1
  2. R. P. Lin, B. R. Dennis, G. J. Hurford, D. M. Smith, A. Zehnder, P. R. Harvey et al.
    Pages 3-32
  3. D. M. Smith, R. P. Lin, P. Turin, D. W. Curtis, J. H. Primbsch, R. D. Campbell et al.
    Pages 33-60
  4. G. J. Hurford, E. J. Schmahl, R. A. Schwartz, A. J. Conway, M. J. Aschwanden, A. Csillaghy et al.
    Pages 61-86
  5. M. Fivian, R. Hemmeck, A. McHedlishvili, A. Zehnder
    Pages 87-99
  6. G. J. Hurford, D. W. Curtis
    Pages 101-113
  7. D. W. Curtis, P. Berg, D. Gordon, P. R. Harvey, D. M. Smith, A. Zehnder
    Pages 115-124
  8. Mark L. McConnell, James M. Ryan, David M. Smith, Robert P. Lin, A. Gordon Emslie
    Pages 125-142
  9. Pascal Saint-Hilaire, Christoph Von Praun, Etzard Stolte, Gustavo Alonso, Arnold O. Benz, Thomas Gross
    Pages 143-164
  10. R. A. Schwartz, A. Csillaghy, A. K. Tolbert, G. J. Hurford, J. McTiernan, D. Zarro
    Pages 165-191
  11. Markus J. Aschwanden, Ed Schmahl, Rhessi Team
    Pages 193-211
  12. Linhui Sui, Gordon D. Holman, Brian R. Dennis, Säm Krucker, Richard A. Schwartz, Kim Tolbert
    Pages 245-259
  13. N. Vilmer, S. Krucker, R. P. Lin, RHESSI Team
    Pages 261-272
  14. E. J. Schmahl, G. J. Hurford
    Pages 273-286
  15. Pascal Saint-Hilaire, Arnold O. Benz
    Pages 287-306
  16. L. Fletcher, H. S. Hudson
    Pages 307-321
  17. David Alexander, Thomas R. Metcalf
    Pages 323-340
  18. Peter T. Gallagher, Brian R. Dennis, Säm Krucker, Richard A. Schwartz, A. Kimberley Tolbert
    Pages 341-356

About this book

Introduction

The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) satellite was launched on 5 February 2002. Its objective is to study the energy release and particle acceleration in solar flares through observations of X-rays and gamma rays. Two novel technologies are combined to obtain both spectra and images over a broad energy range. For the spectroscopy, cooled hyperpure germanium detectors are used to cover the energy range from 3 keV to 17 MeV with unprecedented keV-class resolution. Since focusing optics are not possible for making images with such high energy photons, tungsten and molybdenum absorbing grids are used to modulate the X-rays and gamma-rays coming from the Sun as the spacecraft rotates. This allows the spatial Fourier components of the source to be determined so that images can be made in spectral ranges where astronomical images have never been produced before. These new instrumental techniques require equally innovative software to reconstruct X-ray and gamma-ray spectra and images from the observations.
Ample solar activity, abundant observations, and an open data policy have attracted many researchers. Astronomers face in the RHESSI mission an exciting new scientific potential. It has unusually broad possibilities for improving our understanding of the enigmatic solar flare phenomenon that is becoming increasingly important as society depends more and more on space-based technologies.
In this volume, the functioning of RHESSI is explained, the data analysis techniques including spectroscopy and image reconstruction are introduced, and the experiences of the first few months of operation are summarized. First scientific results are presented that provide the essential base for more extended studies using RHESSI data and complementary observations by instruments on other spacecraft and at ground-based solar observatories.
Scientists and students will find here the latest discoveries in solar flare research, as well as inspiration for future work. The papers will serve as references for the many new discoveries to come from the continuing RHESSI observations.

Keywords

Solar flare instruments observatory solar solar activity spectroscopy sun

Editors and affiliations

  • Robert P. Lin
    • 1
  • Brian R. Dennis
    • 2
  • Arnold O. Benz
    • 3
  1. 1.Space Sciences Laboratory and Physics DepartmentUniversity of CaliforniaBerkeleyUSA
  2. 2.Laboratory for Astronomy and Solar PhysicsNASA Goddard Space Flight CenterGreenbeltUSA
  3. 3.Institute of AstronomyETH-ZentrumZürichSwitzerland

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-017-3452-3
  • Copyright Information Springer Science+Business Media B.V. 2003
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-90-481-6212-3
  • Online ISBN 978-94-017-3452-3
  • About this book