Phase diverse speckle inversion applied to data from the Swedish 1-meter solar telescope

Details Phase diverse speckle inversion applied to data from the Swedish 1-meter solar telescope Phase diverse speckle inversion applied to data from the Swedish 1-meter solar telescope

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4853..567l&link_type=abstract

Innovative Telescopes and Instrumentation for Solar Astrophysics. Edited by Stephen L. Keil, Sergey V. Avakyan . Proceedings o

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

We report on the use of a new joint phase diverse speckle code, an implementation of a method where a single object and individual phases are estimated from several pairs of phase diverse data. The code was used on 430.5 nm G-band data collected with the newly installed Swedish 1-meter solar telescope in La Palma, equipped with a low-order adaptive optics system. We describe the algorithm briefly, show wavefront statistics and object estimates from the processing and discuss the results. We demonstrate a resolution of 0.12 arc seconds for a time sequence and a large field of view, which is a break-through for ground based solar telescopes.

Affiliated with

Also associated with

No associations

Rating

Phase diverse speckle inversion applied to data from the Swedish 1-meter solar telescope 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 Phase diverse speckle inversion applied to data from the Swedish 1-meter solar telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Phase diverse speckle inversion applied to data from the Swedish 1-meter solar telescope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-917187