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EUV Spectroscopy of the Sunspot Region NOAA 7981 Using SOHO - I. Line Emission and Time Dependence
DOI: 10.1023/A:1005003407826 Bibcode: 1998SoPh..179...43B

Harrison, R. A.; Wilhelm, K.; Fredvik, T. +8 more

EUV spectra of a medium-size sunspot and its surroundings, NOAA 7981, were obtained on 2 August 1996 with the Coronal Diagnostic Spectrometer (CDS) and the Solar Ultraviolet Measurements of Emitted Radiation (SUMER) on the Solar and Heliospheric Observatory (SOHO). The spectral lines formed in the transition region and corona show considerable str…

1998 Solar Physics
SOHO 15
Physical properties of the quiescent prominence of 5June 1996, from Hα observations
DOI: 10.1023/A:1005060613653 Bibcode: 1998SoPh..183..323L

Schmieder, B.; Roudier, Th.; Malherbe, J. -M. +2 more

The Multichannel Subtractive Double Pass spectrograph (MSDP) is designed to observe line profiles in a 2D field of view with a good spatial and temporal resolution. In order to deal with this unique opportunity, we introduce a new method for fitting the hydrogen Hα line formed in prominences and deriving various plasma parameters from line profile…

1998 Solar Physics
SOHO 12
The Search for Solar Gravity-Mode Oscillations in the Solar Wind Using it Ulysses Plasma Data
DOI: 10.1023/A:1005034632554 Bibcode: 1998SoPh..179..167H

Riley, Pete; Hoogeveen, Gary W.

A recent report that energetic particles measured in the solar wind may be influenced by solar gravity-mode (-mode) oscillations motivated the search for -mode signatures in the Ulysses solar wind plasma data. Ulysses solar wind plasma data from 1 March 1992 through the 12 April 1996 were examined in this study for signs of possible solar oscillat…

1998 Solar Physics
Ulysses 10
EUV Full-Sun Imaging and Pointing Calibration of the SOHO Coronal Diagnostic Spectrometer
DOI: 10.1023/A:1004915531252 Bibcode: 1998SoPh..178...71T

Thompson, William; Carter, Martin

Although the field of view of the Normal Incidence Spectrometer (NIS) of the Coronal Diagnostic Spectrometer (CDS) is 4×4 arc min, it is possible to observe the full solar disk by forming a mosaic of images taken in succession. This paper describes just such a study which has been used to collect images of the Sun simultaneously in six wavelengths…

1998 Solar Physics
SOHO 6
Ultraviolet Observations of a Dynamic Event in the Solar Corona
DOI: 10.1023/A:1005059530415 Bibcode: 1998SoPh..181..103I

Dwivedi, B. N.; Wilhelm, K.; Curdt, W. +1 more

The Solar Ultraviolet Measurements of Emitted Radiation instrument (SUMER) observations show high Doppler shifts and temporal variations in profiles of ultraviolet lines from low temperature gas in the corona above the active region NOAA 7974. The profiles indicate ≈ 100 km s-1 flows coming from an almost stationary source that appears …

1998 Solar Physics
SOHO 4
Visualization of three-dimensional datasets
DOI: 10.1023/A:1005059601921 Bibcode: 1998SoPh..181...87I

Walsh, Robert W.; Ireland, Jack; Galsgaard, Klaus

The effective visualization of three-dimensional (3d) datasets, both observationally and computationally derived, is an increasing problem in solar physics. We present here plots of computational data derived from the 3d reconstruction of the magnetic field of a loop system, rendered as anaglyphs. By combining images of the same 3d object from two…

1998 Solar Physics
SOHO 1