Abstract
The instruments on the Spartan 201 spacecraft are an Ultraviolet Coronal Spectrometer and a White Light Coronagraph. Spartan 201 was deployed by the Space Shuttle on 11 April 1993 and observed the extended solar corona for about 40 hours. The Ultraviolet Coronal Spectrometer measured the intensity and spectral line profile of HI Lyα and the intensities of OVI 103.2 and 103.7 nm. Observations were made at heliocentric heights between 1.39 and 3.5 R⊙. Four coronal targets were observed, a helmet streamer at heliographic position angle 135°, the north and south polar coronal holes, and an active region above the west limb. Measurements of the HI Lyα geocorona and the solar irradiance were also made. The instrument performed as expected. Straylight suppression, spectral focus, radiometric sensitivity and background levels all appear to be satisfactory. The uv observations are aimed at determining proton temperatures and outflow velocities of hydrogen, protons and oxygen ions. Preliminary results from the north polar coronal hole observations are discussed.
Similar content being viewed by others
References
Esser, R.: 1993, , Personal Communication
Fisher, R. and Guhathakurta, M.: 1993, , Personal Communication
Gouttebroze, P., Lemaire, P., Vial, J. C., and Artzner, G.: 1978,Astrophysical Journal 225, 655
Scudder, J. D.: 1992,Astrophysical Journal 398, 319
Strachan, L., et al.: 1993,Astrophysical Journal 412, 410
Strachan, L., Gardner, L.D., Hassler, D. M. and Kohl, J. L.: 1994,Space Science Rev., this issue
Withbroe, G. L., Kohl, J. L., Weiser, H., and Munro, R. H.: 1982,Space Science Reviews 33, 17
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Kohl, J.L., Gardner, L.D., Strachan, L. et al. Ultraviolet spectroscopy of the extended solar corona during the Spartan 201 mission. Space Sci Rev 70, 253–261 (1994). https://doi.org/10.1007/BF00777876
Issue Date:
DOI: https://doi.org/10.1007/BF00777876