The Level 1C limb data is sampled on a uniform angular grid Latitude.
The data is resampled as follows:
* About 4 scan mirror positions to fill the 0.2° L1C bin.
* Narrow slit width: 0.075°
* Use center of L1B and L1C bins to resample (nearest neighbor) GOLD Public Science Data Products Guide (1.0) 26
* Spectral data is combined within a L1C bin WITHOUT doing any wavelength alignment
for each L1B sample
* 30 bins Altitude
* 32 bins N-S
Version:2.3.1
The Level 1C limb data is sampled on a uniform angular grid Latitude.
The data is resampled as follows:
* About 4 scan mirror positions to fill the 0.2° L1C bin.
* Narrow slit width: 0.075°
* Use center of L1B and L1C bins to resample (nearest neighbor) GOLD Public Science Data Products Guide (1.0) 26
* Spectral data is combined within a L1C bin WITHOUT doing any wavelength alignment
for each L1B sample
* 30 bins Altitude
* 32 bins N-S
| Role | Person | |
|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Richard.Eastes |
| 2. | MetadataContact | spase://SMWG/Person/James.M.Weygand |
GOLD web page with news and other information.
Eastes, R.W., McClintock, W.E., Burns, A.G. et al. Space Sci. Rev. (2017) vol. 212, pp.383.
FTPS access to Gold Level 1C data
HTTPS access to Gold Level 1C data
TThe Tangent Height Altitude grid values.
The Radial Latitude grid values.
TDB seconds from January 1, 2000, 11:58:55.816 UTC at start of L1B time bin.
UTC date/time string: "2017-06-21T23:46:38.015Z".
The number of L1B dwells in each L1C pixel.
The number of L1B pixels in each L1C pixel.
Per pixel quality flags
The wavelengths at each row.
The co-added raw count data.
The random uncertainty of the raw counts.
The co-added corrected counts.
Systematic uncertainty of the corrected counts.
Random uncertainty of the corrected counts.
The spectral radiance at each grid position.
The spectral radiance systematic uncertainty.
The spectral radiance random uncertainty.
The background counts subtracted in the background correction.
Latitude of the reference point.
Longitude of the reference point.
The tangent height of the pixel center ray from the Earth's crust.
The planar angle between the pixel ray from center and the sun direction.
The planar angle between the pixel ray from center and the spacecraft nadir.
The planar angle between the pixel ray from center and the normal to the reference point.
The planar angle between the sun direction to the reference point and the normal to the reference point.