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"employer": "Global Science and Technology, Inc."
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"alt_text": "Time-stamp slates for these frames, organized by wavelength.",
"width": 1340,
"height": 125,
"pixels": 167500
}
}
],
"extra_data": {}
},
{
"id": 313720,
"url": "https://svs.gsfc.nasa.gov/5042/#media_group_313720",
"widget": "Basic text with HTML",
"title": "",
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"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.",
"items": [],
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{
"id": 313721,
"url": "https://svs.gsfc.nasa.gov/5042/#media_group_313721",
"widget": "Basic text",
"title": "For More Information",
"caption": "",
"description": "See [NASA.gov](https://blogs.nasa.gov/solarcycle25/2022/10/03/sun-releases-strong-solar-flare-2)",
"items": [],
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"studio": "svs",
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"credits": [
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"role": "Visualizer",
"people": [
{
"name": "Tom Bridgman",
"employer": "Global Science and Technology, Inc."
}
]
},
{
"role": "Producer",
"people": [
{
"name": "Scott Wiessinger",
"employer": "KBR Wyle Services, LLC"
}
]
},
{
"role": "Technical support",
"people": [
{
"name": "Laurence Schuler",
"employer": "ADNET Systems, Inc."
},
{
"name": "Ian Jones",
"employer": "ADNET Systems, Inc."
}
]
}
],
"missions": [
"SDO"
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"series": [],
"tapes": [],
"papers": [],
"datasets": [
{
"name": "304 Filter",
"common_name": "AIA 304",
"platform": "SDO",
"sensor": "AIA",
"type": "Other",
"organizations": [
"JOINT SCIENCE OPERATIONS CENTER "
],
"description": "",
"credit": "",
"url": "http://jsoc.stanford.edu/",
"date_range": "2022-10-02T18:00UTC - 2022-10-02T22:00UTC"
},
{
"name": "171 Filter",
"common_name": "AIA 171",
"platform": "SDO",
"sensor": "AIA",
"type": "Other",
"organizations": [
"JOINT SCIENCE OPERATIONS CENTER "
],
"description": "",
"credit": "",
"url": "http://jsoc.stanford.edu/",
"date_range": "2022-10-02T18:00UTC - 2022-10-02T22:00UTC"
},
{
"name": "131 Filter",
"common_name": "AIA 131",
"platform": "SDO",
"sensor": "AIA",
"type": "Other",
"organizations": [
"JOINT SCIENCE OPERATIONS CENTER "
],
"description": "",
"credit": "",
"url": "http://jsoc.stanford.edu/",
"date_range": "2022-10-02T18:00UTC - 2022-10-02T22:00UTC"
}
],
"nasa_science_categories": [
"Sun"
],
"keywords": [
"Corona",
"Earth Science",
"EUV Imaging",
"Extreme Ultraviolet Imaging",
"Heliophysics",
"Point-Spread-Function (PSF)",
"SDO",
"Solar Activity",
"Solar Cycle 25",
"Solar Dynamics Observatory",
"Solar Flares",
"Solar Wind",
"Space Weather",
"Sun-earth Interactions"
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"recommended_pages": [],
"related": [],
"sources": [],
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}