Appendix of Solar Surface Source Information |
| Column 1: | '
CME appearance time in LASCO/C2 FOV. Basically, the time from
the SOHO LASCO CME CATALOG are used.
For the CME observed by only STEREO time is used by STEREO-A/B COR1 FOV and
is superseded with *.
|
| Column 2: |
Start time of solar source activity. In case of filament eruption,
basically fast rise time is noted.
|
| Column 3: |
Peak X-ray class of solar source.
|
| Column 4: |
solar source Location.
|
| Column 5: |
If solar source occurs at an active region, note the NOAA active region number.
|
| Column 6: |
If solar source occurs at an active region, active region flux.
|
| Column 7: |
Time to measure the physical quantity of the post eruption arcade.
|
| Column 8: |
Area size underneath the post eruption arcade.
|
| Column 8: |
Average absolute magnetic field strength of the post eruption arcade area.
|
| Column 9: |
Reconnection flux of the post eruption arcade area. It is already divided by 2.
Link to image of the solar source with two arcade footpoint lines (red) and
the arcade tilt line (green).
|
| Column 10: |
Tilt angle of the post eruption arcade at the measurement time.
Does not match the tilt angle of magnetic neutral line. If parallel to the lines of
longitude/latitude, the tite angle is 0/90 degree. The line rising to the right/left
is a positive/negative value.
|
| Column 11: |
Event remarks.
|
| Movie: |
Solar source movie used by SDO HMI and AIA/193. Plotting the arcade footpoint lines
(green) and the magnetic neutral line (pink). |