Artzner, G. E.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Brunaud, J.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Gabriel, Alan H.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Hochedez, J.-F.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Millier, F.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Song, X. Y.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Au, B.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Dere, K. P.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Howard, R. A.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Kreplin, R.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Michels, D. J.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Moses, J. D.[Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
Defise, Jean-Marc[Université de Liège - ULg > > CSL (Centre Spatial de Liège) - Instrumentation et expérimentation spatiales >]
Jamar, Claude[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Rochus, Pierre[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Chauvineau, J.-P.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Marioge, J.-P.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Catura, R. C.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Lemen, J. R.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Shing, L.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Stern, R. A.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Gurman, J. B.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Neupert, W. M.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
Maucherat, A.[Observatoire Royal de Belgique, B-1180 Brussels, Belgium]
1st Advances in Solar Physics Euroconference. Advances in Physics of Sunspots
118
268
Yes
International
[en] SOLAR CORONA ; EXTREME ULTRAVIOLET ; SOHO ; EIT
[en] The Extreme-UV Imaging telescope has already produced more than 15000 wide-field images of the corona and transition region, on the disk and up to 1.5R_o above the limb, with a pixel size of 2.6\arcsec. By using four different emission lines, it provides the global temperature distribution in the quiet corona, in the range 0.5 to 3*E(6) K. Its excellent sensitivity and wide dynamic range allow unprecedented views of low emission features, even inside coronal holes. Those so-called ``quiet'' regions actually display a wide range of dynamical phenomena, in particular at small spatial scales and at time scales going down to only a few seconds, as revealed by all EIT time sequences of full- or partial-field images. The initial results presented here demonstrate the importance of this wide-field imaging experiment for a good coordination between SOHO and ground-based solar telescopes, as well as for science planning.