The LWR ripple correction described in section 11.2.1 of the NEWSIPS image processing manual was modified shortly after the Goddard images had been processed. The new correction derived by Cassatella  slightly improves the ripple correction shortward of 2200 Angstroms. The new correction was implemented at Vilspa and, in Novemeber, 1997, all the Goddard LWR images were reprocessed with the new correction. As a result, all archived LWR high dispersion NEWSIPS data requested after November 14th, 1997 use the ripple correction described below.
The new LWR ripple correction uses the same expression for the parameter as defined in Section 11.2.1 of the NEWSIPS manual. The blaze wavelength for order m however is now defined as:
K = A + Bm + Cm2 + Dm3 + Em4and
A = 0.281749635D+06
B = -0.223565585D+04
C = 0.365319482D+02
D = -0.262477775D+00
E = 0.701464055D-03
The term is a time-dependent correction to the blaze wavelength defined by the equation
where date is the observation date as a fractional year (e.g., 1987.1), and the coefficients are defined at the reference orders shown below.
In practice, the term is calculated at the reference orders for a given observation date and then linearly interpolated to the desired order. Orders longward of order 115 use the correction for order 115, and similiarly orders shortward of order 79 use the correction for order 79.
The study by Cassatella  determined that the changes to the LWR ripple correction did not affect any other calibrations (e.g., the absolute calibration). Therefore, no other calibrations were modified.
To verify images have been processed using the correct ripple correction, a line was added to the HISTORY portion of the primary FITS header. Images processed with the original ripple correction will contain the comment: "LWR RIPPPLE CORRECTION VERSION 1.0 APPLIED". Reprocessed images will have the comment: "LWR RIPPPLE CORRECTION VERSION 2.0 APPLIED".
Note that because the LWR images had already been processed, the LWR ripple correction was applied (at Goddard) using an IDL routine called MXCOR2. The program basically read the net flux vector from the archived MXHI files, re-applied the ripple and absolute flux calibrations, wrote the new ripple-corrected and absolutely-calibrated net flux vectors back into the MXHI file, and updated the comment in the HISTORY portion of the FITS header. At Vilspa, the new correction was implemented in the NEWSIPS processing software. Tests showed the two methods produced identical results.