Several impressive filament eruptions leading up to an M 8.7 Flare at Active Region 13234 - February 27-28, 2023
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- Visualizations by:
- Tom Bridgman
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- Produced by:
- Scott Wiessinger
- View full credits
Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.
Some impressive filaments erupt on the solar limb (lower left and lower right) in the early part of this image series.
Later (17:46:42 TAI), an active region in the upper right quadrant of the solar disk launches a mid-level M 8.7 class flare.Event Description
Some impressive filaments erupt on the solar limb (lower left and lower right) in the early part of this image series.
Later (17:46:42 TAI), an active region in the upper right quadrant of the solar disk launches a mid-level M 8.7 class flare.Event Description
What is the PSF (Point Spread-Function)?
Many telescopes, especially reflecting telescopes such as the ones used on SDO (Wikipedia), have internal structures that support various optical components. These components can result in incoming light being scattered to other parts of the image. This can appear in the image as a faint haze, brightening dark areas and dimming bright areas. The point-spread function (Wikipedia) is a measure of how light that would normally be received by a single camera pixel, gets scattered onto other pixels. This is often seen as the "spikes" seen in images of bright stars. For SDO, it manifests as a double-X shape centered over a bright flare (see Sun Emits Third Solar Flare in Two Days). The effect of this scattered light can be computed, and removed, by a process called deconvolution (Wikipedia). This is often a very compute-intensive process which can be sped up by using a computers graphics-processing unit (GPU) for the computation.Credits
Please give credit for this item to:
NASA's Scientific Visualization Studio
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Visualizer
- Tom Bridgman (GST) [Lead]
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Producer
- Scott Wiessinger (KBR Wyle Services, LLC) [Lead]
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Technical support
- Ian Jones (ADNET Systems, Inc.)
- Laurence Schuler (ADNET Systems, Inc.)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Datasets used in this visualization
SDO AIA 131 (A.K.A. 131 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER
2023-02-27T22:00:00 - 2023-02-28T08:00:00
Dataset can be found at: http://jsoc.stanford.edu/
See more visualizations using this data setSDO AIA 171 (A.K.A. 171 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER
2023-02-27T22:00:00 - 2023-02-28T08:00:00
Dataset can be found at: http://jsoc.stanford.edu/
See more visualizations using this data setSDO AIA 304 (A.K.A. 304 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER
2023-02-27T22:00:00 - 2023-02-28T08:00:00
Dataset can be found at: http://jsoc.stanford.edu/
See more visualizations using this data setNote: 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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