Tag Archives: coronal modeling
180. A global coronal MHD simulation using the HMI vector-magnetic-field synoptic maps
100. Observationally Quantified Reconnection Providing a Viable Mechanism for Active Region Coronal Heating
33. Comparing nonlinear force-free and potential field modeling using full-disk HMI data
16. Spatial-Variance Magnetic Synoptic Maps
Bertello and collaborators at NSO have made a first attempt to estimate some of the uncertainties in magnetic synoptic maps and evaluated their impact on coronal and heliospheric models. They found that accounting for the statistical uncertainties arising from the distribution of image pixels contributing to each bin in the synoptic map may produce a noticeable change in the results obtained from these models.