The wavelength vector as generated by the program
STACK. The vector is linearized to have an increment
of 0.01 angstroms. The minimum and maximum wavelength of the individual scans
determines the wavelength range. All wavelengths are in the heliocentric
coadded background vector corrected for sensitivity degradation.
The vector provided by the OAO-3 project is used by default. If not
available, a background is derived from a table of standard backgrounds
stored as a function of orbit number.
This document was compiled by the
Archive Project. Project members include staff from the GSFC Laboratory
for Astronomy and Solar Physics
(LASP) and the GSFC
Astrophysics Data Facility