High-resolution imaging of the upper solar chromosphere: First light performance of the very-high-resolution Advanced Ultraviolet Telescope

被引:36
作者
Korendyke, CM [1 ]
Vourlidas, A
Cook, JW
Dere, KP
Howard, RA
Morrill, JS
Moses, JD
Moulton, NE
Socker, DG
机构
[1] USN, Res Lab, EO Hulburt Ctr Space Res, Washington, DC 20375 USA
[2] George Mason Univ, Ctr Earth Observing & Space Res, Fairfax, VA 22030 USA
[3] Lab Phys Sci, College Pk, MD 20740 USA
基金
美国国家航空航天局;
关键词
D O I
10.1023/A:1010310217570
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Very-high-resolution Advanced ULtraviolet Telescope (VAULT) experiment was successfully launched on 7 May 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 two-grating, zero-dispersion spectroheliograph tuned to isolate the solar L alpha emission line. During the flight, the instrument successfully obtained a series of images of the upper chromosphere with a limiting resolution of similar to0.33 arc sec. The resulting observations are the highest-resolution images of the solar atmosphere obtained from space to date. The flight demonstrated that sub-arc 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.
引用
收藏
页码:63 / 73
页数:11
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