Physics
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.118a2089s&link_type=abstract
Journal of Physics: Conference Series, Volume 118, Issue 1, pp. 012089 (2008).
Physics
Scientific paper
This investigation aims to study the correlation of the solar background with atmosphere. We used high resolution observations of the NaDl spectral line. In fact the large span in formation heights of this spectral line allowed us to infer the signal from photosphere to chromosphere. We analyzed the data by applying the SIR code (Stokes Inversion based on response functions). It is an inversion method of the RTE (Radiative transfer equation) that provides physical information on the region where the spectral lines are sensitive to changes in thermal and dynamical parameters of the atmosphere. The survey has been divided in two different steps: 1) identification of a model of the atmosphere that reproduce our observations; 2) determination of the degree of correlation of convective motions with the solar atmosphere. Here we present the results of the first step: we identified in the model presented by Vernazza the best model that matches our observations.
Garcia Rafael A.
Jiménez-Reyes Sebastián J.
Pallé Pere Lluis
Ruiz-Cobo B.
Simoniello Rosaria
No associations
LandOfFree
Preliminary results on the contribution of the convection motions to the Doppler velocity signal 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 Preliminary results on the contribution of the convection motions to the Doppler velocity signal, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Preliminary results on the contribution of the convection motions to the Doppler velocity signal will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-853553