Found 12 datasets matching filters.
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\n GOLD retrieves the exospheric temperature from the integrated N2 LBH radiance profile \n obtained from atmospheric limb scans (LIM observation mode). This data product, referred to as...
Search relevance: 1.00 | Views last month: 1 | Published on: 2026-04-13 -
The Level 1C Dayside Disk Images are interrupted via stored instrument commands when \n target stars suitable for occultation measurements approach either limb. \n To perform the occultation...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
The GOLD night disk scan (NI1) measurements are used to derive the peak electron density (NMAX, electrons/cm3) on the disk. GOLD performs NI1 scans in both hemispheres from 17:00 to 21:00 hours...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
The Level 1C Day Disk data is sampled on a uniform angular grid of 0.2° in both Longitude and Latitude. The data is resampled as follows:\n * About 4 scan mirror positions to fill the 0.2° L1C...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
The Level 1C NI1 data is sampled on a uniform angular grid of 0.15° in both Longitude and Latitude. The data is resampled as follows:\n * About 4 scan mirror positions to fill the 0.15° L1C...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
The GOLD daytime disk scan measurements are used to derive the TDISK data product, which is the effective disk neutral temperature at a height of approximately 150 km. TDISK is derived for each...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
GOLD daytime disk scan (DAY) measurements are used to derive the ratio of the column abundance of thermospheric O relative to N2, conventionally referred to as O/N2 or ΣO/N2, but abbreviated to...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
O2 is derived from measurements of stellar occultation in the Shumann Runge continuum. \n As the star rises or sets relative to the satellite position the stellar spectrum is measured across \n ...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
The Level 1C limb data is sampled on a uniform angular grid Latitude. \n The data is resampled as follows:\n * About 4 scan mirror positions to fill the 0.2° L1C bin.\n * Narrow slit width:...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
The GOLD solar irradiance proxy (QEUV) is a proxy for the integrated solar EUV \n irradiance below 45 nm, which can be derived directly from far ultraviolet (FUV) radiance \n measurements....
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
The Level 1C German Space Agency Disk data is sampled on a uniform angular grid of 0.2° in both Longitude and Latitude. The data is resampled as follows:\n * About 4 scan mirror positions to fill...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13 -
O2 is derived from measurements of stellar occultation in the Shumann Runge continuum. \n As the star rises or sets relative to the satellite position the stellar spectrum is measured across \n ...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-13
