Abstract. High-resolution ultraviolet observations of the Sun from SOHO and TRACE spacecraft have provided a wealth of new information on plasma temperature, density, abundance anomaly, plasma flows, turbulence, wave motions, etc., in various solar structures. We briefly present solar physics research of our group, and review some of the new results from the SUMER spectrograph on the SOHO spacecraft, especially the widths of vacuum ultraviolet spectral lines in the equatorial solar corona observed with CDS and SUMER
We present a spectral atlas of the solar corona in the far-ultraviolet (FUV) and extreme ultraviolet...
The scientific goal of UVCS is to obtain detailed empirical descriptions of the extended solar coron...
We present an analysis of 14 ultraviolet emission lines belonging to different atoms and ions observ...
Brightness variations of solar features are investigated using time series of images and spectra of...
Brightness variations of solar features are investigated using time series of images and spectra of...
Brightness variations of solar features are investigated using time series of images and spectra of...
The SUMER (solar ultraviolet measurements of emitted radiation) experiment is described. It will stu...
A far-ultraviolet and extreme-ultraviolet (FUV, EUV) spectral atlas of the Sun between 670 Å and 160...
A far-ultraviolet and extreme-ultraviolet (FUV, EUV) spectral atlas of the Sun between 670 Å and 160...
We analyze a series of full-Sun observations, which was performed with the SoHO/SUMER instrument bet...
The scientific goal of UVCS is to obtain detailed empirical descriptions of the extended solar coron...
The SOHO Ultraviolet Coronagraph Spectrometer is being developed for spectroscopic determinations of...
We present a spectral atlas of the solar corona in the far-ultraviolet (FUV) and extreme ultraviolet...
We present a spectral atlas of the solar corona in the far-ultraviolet (FUV) and extreme ultraviolet...
The scientific goal of Ultraviolet Coronagraph Spectrometer (UVCS) is to obtain detailed empirical d...
We present a spectral atlas of the solar corona in the far-ultraviolet (FUV) and extreme ultraviolet...
The scientific goal of UVCS is to obtain detailed empirical descriptions of the extended solar coron...
We present an analysis of 14 ultraviolet emission lines belonging to different atoms and ions observ...
Brightness variations of solar features are investigated using time series of images and spectra of...
Brightness variations of solar features are investigated using time series of images and spectra of...
Brightness variations of solar features are investigated using time series of images and spectra of...
The SUMER (solar ultraviolet measurements of emitted radiation) experiment is described. It will stu...
A far-ultraviolet and extreme-ultraviolet (FUV, EUV) spectral atlas of the Sun between 670 Å and 160...
A far-ultraviolet and extreme-ultraviolet (FUV, EUV) spectral atlas of the Sun between 670 Å and 160...
We analyze a series of full-Sun observations, which was performed with the SoHO/SUMER instrument bet...
The scientific goal of UVCS is to obtain detailed empirical descriptions of the extended solar coron...
The SOHO Ultraviolet Coronagraph Spectrometer is being developed for spectroscopic determinations of...
We present a spectral atlas of the solar corona in the far-ultraviolet (FUV) and extreme ultraviolet...
We present a spectral atlas of the solar corona in the far-ultraviolet (FUV) and extreme ultraviolet...
The scientific goal of Ultraviolet Coronagraph Spectrometer (UVCS) is to obtain detailed empirical d...
We present a spectral atlas of the solar corona in the far-ultraviolet (FUV) and extreme ultraviolet...
The scientific goal of UVCS is to obtain detailed empirical descriptions of the extended solar coron...
We present an analysis of 14 ultraviolet emission lines belonging to different atoms and ions observ...