Search Publications

The Large Angle Spectroscopic Coronagraph (LASCO)
DOI: 10.1007/BF00733434 Bibcode: 1995SoPh..162..357B

Llebaria, A.; Michels, D. J.; Koomen, M. J. +12 more

The Large Angle Spectroscopic Coronagraph (LASCO) is a three coronagraph package which has been jointly developed for the Solar and Heliospheric Observatory (SOHO) mission by the Naval Research Laboratory (USA), the Laboratoire d'Astronomie Spatiale (France), the Max-Planck-Institut für Aeronomie (Germany), and the University of Birmingham (UK). L…

1995 Solar Physics
SOHO 2638
The Solar Oscillations Investigation - Michelson Doppler Imager
DOI: 10.1007/BF00733429 Bibcode: 1995SoPh..162..129S

Kosovichev, A. G.; Hoeksema, J. T.; Scherrer, P. H. +10 more

The Solar Oscillations Investigation (SOI) uses the Michelson Doppler Imager (MDI) instrument to probe the interior of the Sun by measuring the photospheric manifestations of solar oscillations. Characteristics of the modes reveal the static and dynamic properties of the convection zone and core. Knowledge of these properties will improve our unde…

1995 Solar Physics
SOHO 2267
EIT: Extreme-Ultraviolet Imaging Telescope for the SOHO Mission
DOI: 10.1007/BF00733432 Bibcode: 1995SoPh..162..291D

Michels, D. J.; Gurman, J. B.; Delaboudinière, J. -P. +25 more

The Extreme-ultraviolet Imaging Telescope (EIT) will provide wide-field images of the corona and transition region on the solar disc and up to 1.5 R⊙ above the solar limb. Its normal incidence multilayer-coated optics will select spectral emission lines from Fe IX (171 å), Fe XII (195 å), Fe XV (284 å), and He II (304 å) to provide sensitive tempe…

1995 Solar Physics
SOHO 1687
The SOHO Mission: an Overview
DOI: 10.1007/BF00733425 Bibcode: 1995SoPh..162....1D

Domingo, V.; Fleck, B.; Poland, A. I.

The Solar and Heliospheric Observatory (SOHO) is a space mission that forms part of the Solar-Terrestrial Science Program (STSP), developed in a collaborative effort by the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA). The STSP constitutes the first "cornerstone" of ESA's long-term programme known as "Sp…

1995 Solar Physics
SOHO 1364
SUMER - Solar Ultraviolet Measurements of Emitted Radiation
DOI: 10.1007/BF00733430 Bibcode: 1995SoPh..162..189W

Vial, J. -C.; Grewing, M.; Wilhelm, K. +13 more

The instrument SUMER - Solar Ultraviolet Measurements of Emitted Radiation is designed to investigate structures and associated dynamical processes occurring in the solar atmosphere, from the chromosphere through the transition region to the inner corona, over a temperature range from 104 to 2 × 106K and above. These observat…

1995 Solar Physics
SOHO 837
The Coronal Diagnostic Spectrometer for the Solar and Heliospheric Observatory
DOI: 10.1007/BF00733431 Bibcode: 1995SoPh..162..233H

Mason, H. E.; Harrison, R. A.; Fludra, A. +36 more

The Coronal Diagnostic Spectrometer is designed to probe the solar atmosphere through the detection of spectral emission lines in the extreme ultraviolet wavelength range 150 - 800 å. By observing the intensities of selected lines and line profiles, we may derive temperature, density, flow and abundance information for the plasmas in the solar atm…

1995 Solar Physics
SOHO 648
The Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory
DOI: 10.1007/BF00733433 Bibcode: 1995SoPh..162..313K

Livi, S.; Romoli, M.; Geiss, J. +37 more

The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) is composed of three reflecting telescopes with external and internal occultation and a spectrometer assembly consisting of two toric grating spectrometers and a visible light polarimeter. The purpose of the UVCS instrument is to provide a body of data that can be used to address a broad ra…

1995 Solar Physics
SOHO 457
VIRGO: Experiment for Helioseismology and Solar Irradiance Monitoring
DOI: 10.1007/BF00733428 Bibcode: 1995SoPh..162..101F

Gough, Douglas; Chevalier, André; Domingo, Vicente +22 more

The scientific objective of the VIRGO experiment (Variability of solar IRradiance and Gravity Oscillations) is to determine the characteristics of pressure and internal gravity oscillations by observing irradiance and radiance variations, to measure the solar total and spectral irradiance and to quantify their variability over periods of days to t…

1995 Solar Physics
SOHO 295
Global Oscillations at Low Frequency from the SOHO Mission (GOLF)
DOI: 10.1007/BF00733427 Bibcode: 1995SoPh..162...61G

Damé, L.; García, R. A.; Pallé, P. L. +28 more

The GOLF experiment on the SOHO mission aims to study the internal structure of the sun by measuring the spectrum of global oscillations in the frequency range 10−7 to 10−2 Hz. Bothp andg mode oscillations will be investigated, with the emphasis on the low order long period waves which penetrate the solar core. The instrument…

1995 Solar Physics
SOHO 279
CELIAS - Charge, Element and Isotope Analysis System for SOHO
DOI: 10.1007/BF00733436 Bibcode: 1995SoPh..162..441H

Livi, S.; Hsieh, K. C.; Wurz, P. +30 more

The CELIAS experiment on SOHO is designed to measure the mass, ionic charge and energy of the low and high speed solar wind, of suprathermal ions, and of low energy flare particles. Through analysis of the elemental and isotopic abundances, the ionic charge state, and the velocity distributions of ions originating in the solar atmosphere, the inve…

1995 Solar Physics
SOHO 259