Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..405..311f&link_type=abstract
Solar Polarization 5: In Honor of Jan Stenflo ASP Conference Series, Vol. 405, proceedings of the conference held 17-21 Septembe
Astronomy and Astrophysics
Astronomy
Scientific paper
We have processed full Stokes observations from the SOLIS VSM in the photospheric lines Fe I 630.15 nm and 630.25 nm. The data sets have high spectral and temporal resolution, moderate spatial resolution, and large polarimetric sensitivity and accuracy. We used the LILIA, an LTE code written by \citet{fischer_Navarro2001} to invert the data. We also applied the non-potential magnetic field calculation method of \citet{fischer_Manolis2005} in order to resolve the 180 degree ambiguity. The output are maps of the full magnetic field vector at the photospheric level. Here we present the first inversions of the active region NOAA 10808 during an X-class flare, which occurred on 13 September 2005.
Fischer C. E.
Keller Christoph U.
Snik Frans
No associations
LandOfFree
Vector Magnetic Field Inversions of High Cadence SOLIS-VSM Data 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 Vector Magnetic Field Inversions of High Cadence SOLIS-VSM Data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Vector Magnetic Field Inversions of High Cadence SOLIS-VSM Data will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1068339