KIS H-alpha images from Tenerife


These H alpha images were obtained between 1996 and 2004 during the scientific observation periods with a small auxillary telescope at the Vacuum Tower Telescope (May until December), once per day, if possible.
April 2002: Bandwidth of Lyot filter: now 0.1 nm (before: 0.05 nm).

10. Dezember 2004: Final exposure with the H alpha telescope. This telesope will be replaced during 2006 by ChroTelThe H alpha images obtained so far will still be available via this web-page.


last update: 2006-01-20, hw <hw@kis.uni-freiburg.de>