GREGOR

GFPI Level 1.0 Data on 2017-06-16


Overview of GFPI calibration and Level 0.0 data.

Science Frames

Movie of quick-look GFPI images including: best Broad-Band Image, Full-Width-Half-Minimum, Equivalent Width, Narrow-Band Continuum Image, Narrow-Band Line Core Image and Line-of-Sight Velocity. The time when the data is taken appears below each set of images.

GFPI Camera
Please click on the image to run an AVI movie of all quick-look data from GFPI. Note that quick-look images are not suitable for scientific purposes.

Seeing Conditions

MFGS
The Median Filter Gradient Similarity (MFGS, Deng el al. 2015) is closely related to the seeing conditions under which the data are taken. The red bullets represent the mean value of the MFGS during the image sequence, whereas the blue vertical bars indicate the range between minimum and maximum MFGS values.


Overview of GFPI calibration and Level 0.0 data.

 

Webpage automatically created with sTools (Kuckein et al. 2017) at 16:46:00 UT on 2017-11-10.

The GREGOR solar telescope was built by a German consortium under the leadership of the Kiepenheuer Institute for Solar Physics in Freiburg with the Leibniz Institute for Astrophysics Potsdam, the Institute for Astrophysics Göttingen, and the Max Planck Institute for Solar System Research in Göttingen as partners, and with contributions by the Instituto de Astrofísica de Canarias and the Astronomical Institute of the Academy of Sciences of the Czech Republic.