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"title": "An X1.5 flare and more from Active Region 13664 - May 11, 2024",
"description": "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.An X1.5 flare erupts from Active Region 13664 (lower right quadrant) on May 11, 2024. Less than four hours later, a smaller M8.8 flare erupts from the same region. For more details, see the Space Weather Database for the X1.5 and M8.8 entries. A large filament is also forming on the lower right solar limb.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ",
"release_date": "2024-07-09T00:00:00-04:00",
"update_date": "2024-07-02T10:15:53.260783-04:00",
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"description": "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.
An X1.5 flare erupts from Active Region 13664 (lower right quadrant) on May 11, 2024. Less than four hours later, a smaller M8.8 flare erupts from the same region. For more details, see the Space Weather Database for the X1.5 and M8.8 entries. A large filament is also forming on the lower right solar limb.
For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery.
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What is the PSF (Point Spread-Function)?
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],
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{
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{
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],
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],
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"EUV Imaging",
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}