Coronal heating

Aims:Understand the origin of coronal heating using both observations and theory
   Test the various heating models with coronal observations

Schmieder, B., Rust, D.M., Georgoulis, M.K., Démoulin, P., Bernasconi, P.N.,
                Emerging flux and the heating of coronal loops
         2004, ApJ, 601, 530        PDF
Démoulin P., van Driel-Gesztelyi L., Mandrini C.H., Klimchuk J., Harra L.
                Tests of the coronal heating models using the long-term
                  evolution of AR 7978
         2003, ApJ, 586, n1, March 20    PS gzip
van Driel-Gesztelyi L., Démoulin P., Mandrini C.H., Harra L., Klimchuk J.
                How do the coronal plasma parameters scale with the
                 mean magnetic field? The long-term evolution of AR 7978,
         2003, ApJ, 586, n1, March 20    PS gzip
Mandrini C.H., Démoulin P., KlimchucK J.,
                    Magnetic field and plasma scaling laws:
                        their implications for coronal heating models,
         2000, ApJ 530, 999   PS gzip
Démoulin, P., Priest, E.R.,
                The Importance of Photospheric Intense Flux Tubes for Coronal Heating,
         1997, Solar Physics 175, 123