An X1.9 Class Solar Flare and its Aftermath - January 9, 2023

  • Released Friday, February 10, 2023
  • ID: 5063

The X1.9 flare event of January 9, 2023 as seen in the SDO AIA 131 angstrom filter. Two smaller M-class flares occur at later times on other regions on the solar disk. The dark region around the central 'X' marking the flare is an artifact of the PSF correction. 'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure. Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.



Credits

Please give credit for this item to:
NASA's Scientific Visualization Studio


Missions

This visualization is related to the following missions:

Datasets used in this visualization

SDO AIA 131 (A.K.A. 131 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER 2023-01-09T18:00:00 to 2023-01-10T10:00:00
SDO AIA 171 (A.K.A. 171 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER 2023-01-09T18:00:00 to 2023-01-10T10:00:00
SDO AIA 304 (A.K.A. 304 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER 2023-01-09T18:00:00 to 2023-01-10T10:00:00

Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.


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