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[ascl:1405.007] FORWARD: Forward modeling of coronal observables

FORWARD forward models various coronal observables and can access and compare existing data. Given a coronal model, it can produce many different synthetic observables (including Stokes polarimetry), as well as plots of model plasma properties (density, magnetic field, etc.). It uses the CHIANTI database (ascl:9911.004) and CLE polarimetry synthesis code, works with numerical model datacubes, interfaces with the PFSS module of SolarSoft (ascl:1208.013), includes several analytic models, and connects to the Virtual Solar Observatory for downloading data in a format directly comparable to model predictions.

Code site:
http://people.hao.ucar.edu/sgibson/FORWARD/
Described in:
http://adsabs.harvard.edu/abs/2016FrASS...3....8G http://adsabs.harvard.edu/abs/2014IAUS..300..414F http://adsabs.harvard.edu/abs/2013AGUSMSH51A..02F
Bibcode:
2014ascl.soft05007G

Views: 1542

ascl:1405.007
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