CALIBRATION OF THE SERTS-95 SPECTROGRAPH FROM IRON LINE INTENSITY RATIOS

Goddard Space Flight Center's Solar EUV Rocket Telescope and Spectrogr aph was flown on 1995 May 15 (SERTS-95), carrying a multilayer-coated toroidal diffraction grating which enhanced the instrumental sensitivi ty within its second-order wave band (170-225 Angstrom). Spectra and s pectroheliograms of NOAA Active Region 7870 (N09/W22) were obtained in this wave band with a spectral resolution (instrumental FWHM) similar to 30 m Angstrom. We developed and applied a technique for deriving t he relative radiometric calibration independent of laboratory calibrat ion measurements by employing a method proposed by Neupert & Kastner f or monitoring variations in the sensitivities of orbiting EUV spectrom eters by means of density-and temperature-insensitive Line intensity r atios. Numerous ratios of emission lines from Fe X-XIV are mutually co nsistent and yield an instrumental response curve that matches the des ign characteristics of the multilayer coating. This supports the accur acy of the atomic physics parameters and demonstrates the power of the technique. Many of the ratios employed here can be used to carry out a similar calibration exercise on spectra from the Coronal Diagnostic Spectrometer's Grazing Incidence Spectrograph (CDS/GIS) aboard the Sol ar and Heliospheric Observatory. Because they are relatively free from blending with nearby strong lines, the following density-sensitive ra tios are particularly well suited for analysis with the GIS: Fe X lamb da 175.265/lambda 174.526, Fe X lambda 175.265/lambda 184.534, Fe XII lambda 186.867\lambda 195.117, Fe XIII X203.820/lambda 202.042, Fe XII I lambda 200.017/lambda 202.042, and Fe XIV lambda 219.121/lambda 211. 317. Densities derived from Fe X, XIII, and XIV yield log n(e) similar to 9.3 +/- 0.2.