New requirements for transition region to low corona observations with FUV-EUV spectrometers derived from SOHO experience

被引：0

作者：

Lemaire, P ^{[1
]}

机构：

[1] Univ Paris 11, Inst Astrophys Spatiale, CNRS, Unite Mixte, F-91405 Orsay, France

来源：

CROSSROADS FOR EUROPEAN SOLAR AND HELIOSPHERIC PHYSICS, PROCEEDINGS: RECENT ACHIEVEMENTS AND FUTURE MISSION POSSIBILITIES | 1998年

关键词：

solar high angular resolution; far-extreme ultraviolet emission lines; solar transition zone;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

SOHO FUV-EUV spectrometers are providing an improved understanding of the solar transition region to low corona phenomena. A first analysis of the data obtained shows the observational limitations of the instruments and some related open questions that carl not be answered by the SOHO data. In order to overcome these limitations, to fill new scientific objectives and to provide a reasonable jump in the data quality, we propose new requirements including: angular, spectral and time resolution.

引用

页码：325 / 328

页数：4