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In-flight performance of the Very high Angular Resolution ULtraviolet Telescope sounding rocket payload

  • Clarence M. Korendyke
  • , A. Vourlidas
  • , John W. Cook
  • , Kenneth P. Dere
  • , R. Feldman
  • , Russell A. Howard
  • , D. N. Lilley
  • , Jeff S. Morrill
  • , J. Daniel Moses
  • , Norman E. Moulton
  • , Robert W. Moye
  • , D. E. Roberts
  • , E. L. Shepler
  • , J. K. Smith
  • , Dennis G. Socker
  • , T. R. Spears
  • , R. S. Waymire
  • , Wayne E. Brown
  • , Theodore D. Tarbell
  • , Tom Berger
  • Brian N. Handy
  • Naval Research Laboratory
  • George Mason University
  • Artep Inc
  • University of Maryland, College Park
  • Apogee Instruments
  • Lockheed Martin
  • Montana State University

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

The Very high Angular Resolution ULtraviolet Telescope experiment was successfully launched on May 7, 1999 on a Black Brant sounding rocket vehicle from White Sands Missile Range. The instrument consists of a 30 cm UV diffraction limited telescope followed by a double grating spectroheliograph tuned to isolate the solar Lyman α emission line. During the flight, the instrument successfully obtained a series of images of the upper chromosphere with a limiting resolution of approximately 0.33 arc-seconds. The resulting observations are the highest resolution images of the solar atmosphere obtained from space to date. The flight demonstrated that subarc-second ultraviolet images of the solar atmosphere are achievable with a high quality, moderate aperture space telescope and associated optics. Herein, we describe the payload and its in-flight performance.

Original languageEnglish
Pages (from-to)340-349
Number of pages10
JournalProceedings of SPIE - The International Society for Optical Engineering
Volume4139
DOIs
StatePublished - 2000
Externally publishedYes

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