Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-07-05T17:25:31.179Z Has data issue: false hasContentIssue false
  • English
  • Français

The Integrated Magnetic Field of the Sun Seen by the Golf Experiment

Published online by Cambridge University Press:  08 February 2017

R.A. García ,
T. Roca Cortés  and
The GOLF Team
R.A. García
Affiliation:
SAp, DAPNIA/DSM, CE Saclay. 91191 France
T. Roca Cortés
Affiliation:
Instituto de Astrofisica de Canarias, E-38205, Tenerife, Spain

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The secondary objective of the GOLF experiment on-board the SOHO space mission is to measure the line-of-sight component of the disk averaged magnetic field of the Sun. GOLF is an improved disk-integrated sunlight resonant scattering spectrophotometer. Using an extra fixed quarter wave plate placed at the entrance of the instrument, enables a selection of the circularly polarized solar light and therefore, the disk averaged solar line-of-sight component of the magnetic field can be obtained. Unfortunately, due to occasional malfunction of the rotating mechanisms, only a series of 26 continuous days are available. Here, the analysis of this series is presented including the value of the averaged magnetic field.

Type
IV. Solar Small-Scale Structure
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 225 - 226
Copyright
Copyright © Kluwer 1998 

References

García, R.A., 1996, , Univ. La Laguna, Tenerife, Spain Google Scholar
García, R.A., Roca Cortés, T. and Régulo, C. 1997, Astron. Astrophys. Supp. in Press.Google Scholar
Stix, M. 1989, The Sun. An Introduction, Springer-Verlag Google Scholar