Five times the solar disk in a long row from left to right with main colors orange, light green, blue, green-red sprinkles, blue-to-red gradient, respresenting exemplary PMI data products after on-board analysis from left to right: continuum intensity, magnetic field strength, magnetic field inclination, magnetic field azimuth and line-of-sight velocity.

Publications of R. Muller

Conference Paper (1)

1.
Conference Paper
Damé, L.; Acton, L.; Brunner, M. E.; Connes, P.; Cornwell, T. J.; Curdt, W.; Foing, B. H.; Hammer, R.; Harrison, R.; Heyvaerts, J. et al.; Karabin, M.; Marsch, E.; Martic, M.; Mattig, W.; Muller, R.; Patchett, B.; Cortés, T. R.; Rutten, R. J.; Schmidt, W.; Title, A. M.; Tondello, G.; Vial, J.-C.; Visser, H.: Design rationale of the Solar Ultraviolet Network (SUN). In: Proceedings of the ESO Conference on High Resolution Imaging by Interferometry II, Garching, 15.-18. Oktober 1991. (1991)
MPG.PuRe

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