Abstract
The Preflare Activity Team at the Solar Maximum Mission Workshops was split into three groups. The first group, concerned with Magneto-hydrodynamic Stability (see Section 1.2), was led by E.R. Priest. Its members were A. Aydemir, F. Brunel, P. Cargill, T. Forbes, A. Hood, J. Melville, B. Schmieder, R. Steinolfson, and G. Van Hoven. The second group discussed Preflare Magnetic and Velocity Fields (see Section 1.3). It was led by M. Hagyard and included G. Chapman, A. de Loach, F. Drago, A. Gary, B. Haisch, W. Henze, V. Gaizauskas, H. Jones, J. Karpen, M. Martres, J. Porter, E. Reichmann, B. Schmieder, G. Simon, J. Smith, Jr., and J. Toomre. The third group considered Coronal Manifestations of Preflare Activity (see Section 1.4) under the leadership of E. Schmahl and D. Webb. Its members were R. Bentley, F. Drago, S. Enome, V. Gaizauskas, R. Harrison, G. Hurford, B. Jackson, T. Kosugi, M. Kundu, K. Lang, A. Magun, P. Martens, G. Pneuman, E. Reichmann, A. Schadee, J. Schrijver, B. Schmieder, G. Simon, J. Smith, Jr., K. Strong, P. Waggett and B. Woodgate.
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Priest, E.R., Gaizauskas, V., Hagyard, M.J., Schmahl, E.J., Webb, D.F. (1989). Preflare Activity. In: Kundu, M.R., Woodgate, B., Schmahl, E.J. (eds) Energetic Phenomena on the Sun. Astrophysics and Space Science Library, vol 153. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2331-7_1
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