` Institute for Astrophysics Göttingen

At hh:mm:ss UTC on dd.mm.yyyy the CME is best visible/observable in the Field of View of STEREO/SECCHI/COR2 based on observation with the COR2 synoptic movies.

Download Movie

COR2B white-light Coronagraph image (left), COR2A white-light Coronagraph image (right).

COR2B white-light Coronagraph image with an overlay in green of the GCS wireframe (left),
COR2A white-light Coronagraph image with an overlay in green of the GCS wireframe (right)

The Fitting with the GCS Forward-Modeling Code yields the following results.
GCS Fit-Parameter from Modeling:
Carrington Longitude:
Carrington Latitude:
Tilt Angle:
Height:
Ratio:
Half Angle:
Timestamp of used COR2-Images for Modeling: yyyymmddThhmmss #formatting: yyyymmddThhmmss
EUVI-B image at 195 A on dd.mm.yyyy at hh:mm:ss (left), EUVI-A image at 195 A on dd.mm.yyyy at hh:mm:ss (right)

© Institute for Astrophysics Göttingen