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Solar high resolution balloon spectra obtained in the 190–300 nm wavelength band

  • Posters: High Resolution Techniques of Observation and Data Reduction
  • Conference paper
  • First Online:
High Resolution in Solar Physics

Part of the book series: Lecture Notes in Physics ((LNP,volume 233))

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Abstract

A balloon gondola with a solar telescope spectrograph mounted on an equatorial platform has been launched from Aire/Adour (France) October 1, 1982. High quality spectra with a spectral resolution better than 1.5 pm and with a 4–5. arcseconds angular resolution have been recorded in the atmospheric window domains : 195–212 nm and 272–292 nm. Results from this first flight are discussed.

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Bibliography

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Authors and Affiliations

  1. Laboratoire de Physique Stellaire et Planétaire, B.P. 10 Route des Gatines, 91371, Verrieres Le Buisson Cedex

    D. Samain & P. Lemaire

Authors
  1. D. Samain
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  2. P. Lemaire
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Richard Muller

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© 1985 Springer-Verlag

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Samain, D., Lemaire, P. (1985). Solar high resolution balloon spectra obtained in the 190–300 nm wavelength band. In: Muller, R. (eds) High Resolution in Solar Physics. Lecture Notes in Physics, vol 233. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0022404

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  • DOI: https://doi.org/10.1007/BFb0022404

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-15678-9

  • Online ISBN: 978-3-540-39608-6

  • eBook Packages: Springer Book Archive

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