Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-08-20
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
accepted by ApJL
Scientific paper
The Sunrise balloon-borne solar observatory consists of a 1m aperture Gregory telescope, a UV filter imager, an imaging vector polarimeter, an image stabilization system and further infrastructure. The first science flight of Sunrise yielded high-quality data that reveal the structure, dynamics and evolution of solar convection, oscillations and magnetic fields at a resolution of around 100 km in the quiet Sun. After a brief description of instruments and data, first qualitative results are presented. In contrast to earlier observations, we clearly see granulation at 214 nm. Images in Ca II H display narrow, short-lived dark intergranular lanes between the bright edges of granules. The very small-scale, mixed-polarity internetwork fields are found to be highly dynamic. A significant increase in detectable magnetic flux is found after phase-diversity-related reconstruction of polarization maps, indicating that the polarities are mixed right down to the spatial resolution limit, and probably beyond.
Barthol Peter
Bello González Nazaret
Berkefeld Th.
Bonet Jose Antonio
Danilovic Sanja
No associations
LandOfFree
Sunrise: instrument, mission, data and first results does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Sunrise: instrument, mission, data and first results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sunrise: instrument, mission, data and first results will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-80637