Analysis of transition-region emission-line profiles from full-disk scans of the sun using the SUMER instrument on SOHO

被引:111
作者
Peter, H
机构
[1] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[2] Natl Ctr Atmospher Res, Adv Study Program, Boulder, CO 80307 USA
关键词
solar wind; Sun : transition region;
D O I
10.1086/307102
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine statistical properties of line profiles seen in full-disk observations with the UV spectrograph SUMER on board SOHO. In the SUMER data archive,full-disk data with complete spectral information are available only for wavelength regions including the He I (584 Angstrom), Ne VIII (770 Angstrom), C III (977 Angstrom) and C IV (1548 Angstrom) emission lines. In this paper we will concentrate on C IV and Ne VIII. Collectively these data provide us with the unique opportunity to study the properties of line profiles in the lower and upper solar transition-region beyond what could be achieved with earlier instruments. In particular, these data reveal the center-to-limb behavior of line shifts and line widths for the first time ina statistically meaningful way. For C IV these data show the well-known redshift: of the transition-region lines in the quiet Sun and a clear correlation of the Doppler shift and the nonthermal broadening to the intensity as a characteristic of the network structure. This correlation is not found in the coronal holes. No indications for the network can be found in Ne vm. For Ne VIII we find a center-to-limb variation of the line shift opposite to C IV, which leads to the conclusion that Ne VIII must be blueshifted at disk center. This also shows the need for a remeasurement of the wavelength of Ne VIII in the laboratory. The center-to-limb variation of the line width leads to the conclusion that the nonresolved motions are not isotropic with a preference for the vertical component. Both lines show a clear signal for an outflow in the polar coronal holes. We discuss the implications of these and other observations for models of the transition-region and corona. The line shift behavior of Ne VIII and other lines from the upper transition-region deserves deeper investigation and probably has pivotal importance in our understanding of the solar transition-region. We are pursuing such work.
引用
收藏
页码:490 / 504
页数:15
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