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Hydrodynamics of Flaring Loops: SMM Observations and Numerical Simulations

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Recent Advances in the Understanding of Solar Flares

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Abstract

The hydrodynamic response of confined magnetic structures to strong heating perturbations is investigated by means of a time-dependent one-dimensional code which incorporates the energy, momentum and mass conservation equations. The entire atmospheric structure from the chromosphere to the corona is taken into account. The results of model calculations are compared with observations of flares obtained with the X-Ray Polychromator experiment on the Solar Maximum Mission.

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References

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Author information

Authors and Affiliations

  1. Osservatorio Astrofisico di Arcetri, Firenze, Italy

    R. Pallavicini

  2. Osservatorio Astronomico di Palermo, Italy

    G. Peres

Authors
  1. R. Pallavicini
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  2. G. Peres
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Editor information

Editors and Affiliations

  1. University of California at Berkeley, Berkeley, California, USA

    S. R. Kane

  2. Tokyo Astronomical Observatory, University of Tokyo, Mitaka, Tokyo, Japan

    Y. Uchida  & K. Tanaka  & 

  3. Center for Astrophysics and Space Science, University of California at San Diego, La Jolla, California, USA

    H. S. Hudson

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© 1983 D. Reidel Publishing Company, Dordrecht, Holland

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Pallavicini, R., Peres, G. (1983). Hydrodynamics of Flaring Loops: SMM Observations and Numerical Simulations. In: Kane, S.R., Uchida, Y., Tanaka, K., Hudson, H.S. (eds) Recent Advances in the Understanding of Solar Flares. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7228-5_16

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  • DOI: https://doi.org/10.1007/978-94-009-7228-5_16

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7230-8

  • Online ISBN: 978-94-009-7228-5

  • eBook Packages: Springer Book Archive

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