High-resolution solar polarimetry with Sunrise
Abstract
Sunrise is a solar telescope with an aperture of 1 m, and is dedicated for spectropolarimetric measurements in the visible and the near UV. The total wavelength range is 200 to 1000 nm for narrowband imaging and diagnostic spectroscopy. Sunrise is planned as a stratospheric long-duration balloon mission with a first flight in 2006
- Publication:
-
Astronomische Nachrichten
- Pub Date:
- December 2001
- DOI:
- 10.1002/1521-3994(200112)322:5/6<363::AID-ASNA363>3.0.CO;2-V
- Bibcode:
- 2001AN....322..363S