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 (alpha) 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.
In-flight performance of the Very high Angular resolution ULtraviolet Telescope sounding rocket payload
Instrumentation for UV/EUV Astronomy and Solar Missions ; 2000 ; San Diego,CA,United States
Proc. SPIE ; 4139
2000-12-18
Conference paper
Electronic Resource
English
British Library Conference Proceedings | 2000
|Normal Incidence X-Ray Telescope Sounding Rocket Payload
NTIS | 1987
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