;******************************************************************************* ; Magnification.pro SUMER Magnification Factor and Spectral Resolution Element ; K. W. 05 Jan 1994 ; Rev. 2 (Mean pixel size: 0.0265 mm) 10 Dec 1994 ; Short version 19 Nov 1996 ; Completed for detector B 12 May 1997 ++++ ; Correction detector B 11 Aug. 1998 ???? ; The correction of August 1998 was no improvement 01 Sept. 1998 .... ; Corrected to comply with flight S/W .... ; Mean spectral pixel size: Detector A = 0.0266 mm, Detector B = 0.0265 mm .... ; Mean spatial pixel size: No Change (0.0265 mm for both detectors) .... ; The September 1, 1998 modification changes the original value of .... ; Detector A by 0.38 % (0.0266/0.0265) and of B by 0.18 % at 660 A .... ; and 0.3 % at 1460 A .... ; Separated from Radiometry.pro 26 Nov. 1998 ; Second order dispersion corrected for detector B 07 June 1999 %%%% ; Rev. of second order dispersion for detector B 15 June 1999 %%%% pro magnification,wavelength,order,mag_a,d_lam_a,mag_b,d_lam_b ; ++++ ;------------------------------------------------------------------------------ ; Wavelength in Angstroem ; mag_a: Magnification slit plane/detector plane for detector A ; d_lam_a: Wavelength interval per pixel on detector A in Angstroem ; mag_b: Magnification slit plane/detector plane for detector B ++++ ; d_lam_b: Wavelength interval per pixel on detector B in Angstroem ???? ; Order of diffraction d=2777.45d0 ; in Angstroem, (Grating constant) ra=3200.78 ; in mm, radius of grating fc=399.60 ; in mm, focal length of collimator ; Detector A px_s_a=0.0266 ; in mm .... ; mean spectral pixel size Detector A .... ; mean spatial pixel size for A + B: 0.0265 .... sin_theta=order*wavelength/d cos_theta=sqrt(1-sin_theta^2) f_lambda=ra/(1+cos_theta) mag_a=f_lambda/fc d_lam_a=d*px_s_a/order/f_lambda ; Detector B lambda_n,order*wavelength,lambda_n ; .... %%%% grating_b_511,lambda_n,d_lam_b,mag_b ; .... d_lam_b=d_lam_b/order; %%%% return end