Old and New Aspects of Prominence Physics from Coronal Observations

Details Old and New Aspects of Prominence Physics from Coronal Observations Old and New Aspects of Prominence Physics from Coronal Observations

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..368..331k&link_type=abstract

The Physics of Chromospheric Plasmas ASP Conference Series, Vol. 368, Proceedings of the conference held 9-13 October, 2006 at t

Physics

1

Scientific paper

Classical W-L eclipse observations at typical spatial resolution of 10 arcsec show dark cavities surrounding prominences. Images at higher spatial resolution processed with a spatial filter reveal small dynamical cool clouds moving inside the inner corona around prominences. More recently EIT/SoHO observations taken using the 304 Å channel showed He+ prominences sometimes not seen in cooler lines. TRACE movies of the Fe IX and XI emissions where prominences are seen in absorption also bring appreciable informations on the dynamical surrounding of prominences, without showing obvious correlations between prominence and coronal structures. Accordingly, we re-examine the significance of the cavity and propose a possible interpretation as magnetic interlaced 3-D flux ropes and loops evacuating the corona, in addition to twisted flux ropes where the prominence plasma is condensing. Future space missions like ASPIICS should pay more attention to cavities and emptiness, to coronal dynamics around prominences, in order to resolve the long-standing problem of the origin of prominences and perhaps, perform a new diagnostic of the erupting process responsible for many CMEs.

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