TIMED SEE Level 3 Solar Irradiance Data
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Complete Metadata
| @type | dcat:Dataset |
|---|---|
| accessLevel | public |
| bureauCode |
[ "026:00" ] |
| contactPoint |
{ "fn": "NASA Space Physics Data Facility", "@type": "vcard:Contact", "hasEmail": "mailto:NASA-SPDF-Support@nasa.onmicrosoft.com" } |
| description | SEE Level 3 data files contain one daily averaged solar irradiance spectrum in 1 nm intervals extracted from the EGS Level 2 and XPS Level 2 data products. Shortward of 27 nm, a solar model is scaled to match the XPS broadband data. SEE Level 3 data files also contain 38 emission lines extracted from EGS Level 2 spectra, and the XPS Level 2 diode irradiances. For normal operations, SEE observes the Sun for about 3 minutes every orbit (97 minutes), which usually gives 14-15 measurements per day. The SEE Level 3 data are time averaged over the entire day, after applying corrections for atmospheric absorption, degradation, flare removal, and to 1-AU. |
| distribution |
[ { "@type": "dcat:Distribution", "format": "BIN", "mediaType": "application/octet-stream", "downloadURL": "http://lasp.colorado.edu/home/see/data/" }, { "@type": "dcat:Distribution", "format": "BIN", "mediaType": "application/octet-stream", "downloadURL": "http://lasp.colorado.edu/home/see/data/daily-averages/level-3/" }, { "@type": "dcat:Distribution", "format": "BIN", "mediaType": "application/octet-stream", "downloadURL": "https://helio.data.nasa.gov/dataset/TIMED_SEE_L3" }, { "@type": "dcat:Distribution", "format": "BIN", "mediaType": "application/octet-stream", "downloadURL": "https://hpde.io/NASA/NumericalData/TIMED/SEE/L3" } ] |
| identifier | https://doi.org/10.48322/62p4-es92 |
| keyword |
[ "irradiance", "see", "sun", "timed" ] |
| landingPage | https://doi.org/10.48322/62p4-es92 |
| license | https://www.usa.gov/government-works |
| modified | 2026-08-17 |
| programCode |
[ "026:000" ] |
| publisher |
{ "name": "SEE_POC", "@type": "org:Organization" } |
| theme |
[ "Heliophysics" ] |
| title | TIMED SEE Level 3 Solar Irradiance Data |