SWAN: A study of solar wind anisotropies on SOHO with lyman alfa sky mapping

Jean-Loup Bertaux, Erkki Kyrölä, E. Quemerais, R. Pellinen, R. Lallement, W. Schmidt, Michel Berthe, E. Dimarellis, Jean-Pierre Goutail, C. Taulemesse, C. Bernard, G. Leppelmeier, T. Summanen, Heikki Hannula, Heikki Huomo, Väinö Kelhä, S. Korpela, K. Leppälä, E. Strömmer, J. TorstiKai Viherkanto, J.F. Hochedez, G. Chretiennot, R. Peyroux, T. Holzer

    Research output: Chapter in Book/Report/Conference proceedingChapter or book articleScientificpeer-review

    Abstract

    On board the SOHO spacecraft poised at L1 Lagrange point, the SWAN instrument is mainly devoted to the measurement of large scale structures of the solar wind, and in particular the distribution with heliographic latitude of the solar wind mass flux. This is obtained from an intensity map of the sky Lymanα emission, which reflects the shape of the ionization cavity carved in the flow of interstellar H atoms by the solar wind. The methodology, inversion procedure and related complications are described. The subject of latitude variation of the solar wind is shortly reviewed: earlier Lymanα results from Prognoz in 1976 are confirmed by Ulysses. The importance of the actual value of the solar wind mass flux for the equation of dynamics in a polar coronal hole is stressed. The instrument is composed of one electronic unit commanding two identical Sensor Units, each of them allowing to map a full hemisphere with a resolution of 1°, thanks to a two-mirrors periscope system. The design is described in some details, and the rationale for choice between several variants are discussed. A hydrogen absorption cell is used to measure the shape of the interplanetary Lymanα line and other Lyman α emissions. Other types of observations are also discussed : the geocorona, comets (old and new), the solar corona, and a possible signature of the heliopause. The connexion with some other SOHO instruments, in particular LASCO, UVCS, SUMER, is briefly discussed.
    Original languageEnglish
    Title of host publicationThe SOHO Mission
    EditorsB. Fleck, V. Domingo, A. Poland
    PublisherSpringer
    Pages403-439
    ISBN (Electronic)978-94-009-0191-9
    ISBN (Print)978-94-010-6569-6
    DOIs
    Publication statusPublished - 1995
    MoE publication typeA3 Part of a book or another research book

      Fingerprint

    Cite this

    Bertaux, J-L., Kyrölä, E., Quemerais, E., Pellinen, R., Lallement, R., Schmidt, W., Berthe, M., Dimarellis, E., Goutail, J-P., Taulemesse, C., Bernard, C., Leppelmeier, G., Summanen, T., Hannula, H., Huomo, H., Kelhä, V., Korpela, S., Leppälä, K., Strömmer, E., ... Holzer, T. (1995). SWAN: A study of solar wind anisotropies on SOHO with lyman alfa sky mapping. In B. Fleck, V. Domingo, & A. Poland (Eds.), The SOHO Mission (pp. 403-439). Springer. https://doi.org/10.1007/978-94-009-0191-9