A JSON file can be loaded using PyThea tool (https://www.pythea.org) to visualize the kinematic reconstruction results
along with remote-sensing observations of the Sun and Solar Corona.

Wile using PyThea, the 'Running Fitting Table' provides the fitted parameters of the geometrical model to the selected
image.

The parameters are

HGLN: source longitude in Heliographic coordinate system
HGLT: source latitude in Heliographic coordinate system
CRLN: source longitude in Carrington coordinate systen
CRLT: source lotitude in Carrington coordinate system
RCENTER: distance of the center of the ellipsoid from the center of the Sun (in units of solar radii Rs)
RADAXIS: size of the radial axis of the ellipsoid, a (in units of solar radii Rs)
ORTHOAXIS1: size of first transverse axis of the ellipsoid, b (in units of solar radii Rs)
ORTHOAXIS2: size of second transverse axis of the ellipsoid, c (in units of solar radii Rs)
TILT: tilt angle of the ellipsoid
HEIGHT, KAPPA, EPSILON, ALPHA: ellipsoid parameters (alternative to rcenter, radixis and orthoaxis's definitions)
Imager: reference imager that was used for the fit
Time: time of the fit in UTC
Kinematics: gives the parameters of the smoothing function

These parameters are stored when the user makes a fit using PyThea and presses the 'Store Fit' button. The
'Stored Fitting Table' provides all these fitted parameters of the geometrical model to the various images. The
information in this table updates when a new single fitting is stored. The parameters stored in this table can be
downloaded in a JSON file when the overall fitting of an event is ready from the 'Finalize and save results' section by
pressing the 'Download Fitting as .json file'. Additionally, the user can load the fitting parameters from any of the
single fittings (i.e. rows).

Some explanatory content is available on PyThea webpage:
https://www.pythea.org/en/docs/application.html#the-graphical-user-interface.