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Solar physics at ultrahigh resolution from the space station with the Solar Ultraviolet Network (SUN)

  • L. Damé*
  • , L. Acton
  • , M. Bruner
  • , P. Connes
  • , T. Cornwell
  • , B. Foing
  • , J. Heyvaerts
  • , P. Lemaire
  • , M. Martić
  • , R. Muller
  • , T. Roca Cortés
  • , J. Riehl
  • , R. Rutten
  • , A. M. Title
  • , J. C. Vial
  • , H. Visser
  • , G. Weigelt
  • *Šī darba korespondējošais autors
  • Office national d'études et de recherches aérospatiales
  • Service d'Aéronomie
  • Lockheed Martin
  • National Science Foundation
  • European Space Research and Technology Centre (ESTEC)
  • Observatoire de Paris
  • Université Paris-Saclay
  • Observ. Midi-Pyrénées
  • Instituto de Astrofísica de Canarias
  • Utrecht University
  • Netherlands Organisation for Applied Scientific Research
  • Max Planck Institute for Radio Astronomy

Zinātniskās darbības rezultāts: Devums žurnālamZinātniskais raksts (žurnālā)koleģiāli recenzēts

Kopsavilkums

The SUN experiment is a UV and visible Space Interferometer aimed at ultra-high resolution in the solar atmosphere. It has been proposed to ESA as part of the SIMURIS Mission Proposal which has recently been accepted for an Assessment Study in the framework of the Space Station. The 4 × 20 cm telescopes of the SUN linear array are non-redundantly placed to cover a 2 m baseline, and the instrument makes full use of stabilized interferometry potential, the 4 telescopes being co-aligned and co-phased on a reference field on the sun. After a brief outline of the scientific objectives, the concept of the instrument is described, and its image reconstruction potential is illustrated.

OriģinālvalodaAngļu
Lapas (no-līdz)267-270
Lapu skaits4
ŽurnālsAdvances in Space Research
Sējums11
Izdevuma numurs5
DOIs
Publikācijas statussPublicēts - 1991
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