New observations of the magnetic vector field across the solar disk

C.U. Keller, J.W. Harvey, C.J. Henney

Research output: Chapter in Book/Report/Conference proceedingChapterAcademic

Abstract

Full disk solar magnetograms have been available for more than three decades. However, those maps only show the line-of-sight magnetic flux. The physical quantity we really want to know is the magnetic field vector along with the filling factor, i.e. the fractional area of the resolution element that is occupied by the magnetic field. Since August 2003, the SOLIS Vector-SpectroMagnetograph has been recording the photospheric magnetic field vector across the full solar disk with high sensitivity and resolution. Some of the data are now becoming available for beta testing, and the first science results are emerging. Here we provide a brief introduction to the instrument and its data products and then present some of the data from the first three years of operation.
Original languageUndefined/Unknown
Title of host publication4th Cambridge workshop on cool stars, stellar systems and the sun : proceedings of a workshop held by Spitzer Science Center at Hilton Pasadena Hotel, Pasadena, California, USA 5-10 November 2006
EditorsG. van Belle
Place of PublicationSan Francisco
PublisherAstronomical Society of the Pacific
Pages166-173
Number of pages441
ISBN (Print)978-1-58381-331-7
Publication statusPublished - 2008

Publication series

NameAstronomical Society of the Pacific conference series
Number384

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