High-resolution observations of the extreme ultraviolet sun

被引：78
|
作者：
Harrison, RA
Fludra, A
Pike, CD
Payne, J
Thompson, WT
Poland, AI
Breeveld, ER
Breeveld, AA
Culhane, JL
KjeldsethMoe, O
Huber, MCE
Aschenbach, B
机构：
[1] NASA, GODDARD SPACE FLIGHT CTR, GREENBELT, MD 20771 USA
[2] UCL, MULLARD SPACE SCI LAB, DORKING RH5 6NT, SURREY, ENGLAND
[3] UNIV OSLO, INST THEORET ASTROPHYS, N-0315 OSLO, NORWAY
[4] EUROPEAN SPACE AGCY, DEPT SPACE SCI, NL-2200 AG NOORDWIJK, NETHERLANDS
[5] MAX PLANCK INST EXTRATERR PHYS, D-85748 GARCHING, GERMANY
来源：
SOLAR PHYSICS | 1997年 / 170卷 / 01期
关键词：
Atmosphere; Future Study; Transition Region; Emission Line; Diagnostic Information;
D O I：
10.1023/A:1004913326580
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This paper presents first results of the Coronal Diagnostic Spectrometer (CDS) recently launched aboard the Solar and Heliospheric Observatory (SOHO). CDS is a twin spectrometer, operating in the extreme ultraviolet range 151-785 Angstrom. Thus, it can detect emission lines from trace elements in the corona and transition region which will be used to provide diagnostic information on the solar atmosphere. In this paper, we present early spectra and images, to illustrate the performance of the instrument and to pave the way for future studies.
引用
收藏
页码：123 / 141
页数：19
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