| Zugriffsnummer | 20073 |
| Dokumenttyp | Zeitschriftenartikel |
| Sprache | Englisch |
| Titel | Laboratory calibration of the Extreme-ultraviolet Imaging Spectrometer for the Solar-B satellite |
| Autor(in); Institution |
Lang, J.; Rutherford Appleton Laboratory, Oxfordshire, UK
Kent, B. J.; Rutherford Appleton Laboratory, Oxfordshire, UK
Paustian, Wolfgang; 7.1, Photonenradiometrie, PTB-Berlin
Brown, C. M.; Space Science Division, U.S. Naval Research Laboratory, Washington, D.C., USA
Keyser, Ch.; Space Science Division, U.S. Naval Research Laboratory, Washington, D.C., USA
Anderson, M. R.; Rutherford Appleton Laboratory, Oxfordshire, UK
Case, G. C. R.; Rutherford Appleton Laboratory, Oxfordshire, UK
Chaudry, R. A.; Mullard Space Science Laboratory, University College London, Surrey, UK
James, A. M.; Mullard Space Science Laboratory, University College London, Surrey, UK
Korendyke, C. M.; Space Science Division, U.S. Naval Research Laboratory, Washington, D.C., USA
Pike, C. D.; Rutherford Appleton Laboratory, Oxfordshire, UK
Probyn, B. J.; School of Physics and Space research, The University of Birmingham, Birmingham, UK
Rippington, D. J.; Rutherford Appleton Laboratory, Oxfordshire, UK
Seely, J. F.; Space Science Division, U.S. Naval Research Laboratory, Washington, D.C., USA
Tandy, J. A.; Mullard Space Science Laboratory, University College London, Surrey, UK
Whillock, M. C. R.; Mullard Space Science Laboratory, University College London, Surrey, UK
|
| Quelle/Jahr | Applied Optics: 45 (2006), 34, 8689 - 8705 |
| ISSN | 0003-6935 |
| DOI | |
| URL | |
| Verlag | Washington, DC: Soc. |
| Klassifikationscode | OCIS: 120.5630 ; OCIS: 120.6200 ; OCIS: 300.6540 ; OCIS: 300.6560 ; OCIS: 340.7440 |
| Zusammenfassung | The laboratory end to-end testing of the Extreme-ultraviolet Imaging Spectrometer (EIS) for the Solar-B satellite is reported. A short overview of EIS, which observes in two bands in extreme-ultraviolet wavelength range, is given. The calibration apparatus is described, including details of the light sources used in the work. The data reduction and analysis procedure are outlined. The wavelength calibration using a Penning source to illuminate the aperture fully is presented. A section is devoted to the aperture determination using a radiometrically calibrated hollow cathode based source. The sensitivity section gives an account of the predicted and measured efficiencies from consideration of the efficiencies of individual optical elements in the first order, an account of efficiencies out of band when radiation incident in one band is detected in the other, and efficiencies in multiple orders. The efficiencies measured in the first order both in-band and out of band are compared to the predictions and the sensitivity and its uncertainties are derived. The application of the radiometric calibration is discussed. |
Zitierung
Lang, J., Kent, B. J., Paustian, W., Brown, C. M., Keyser, C., Anderson, M. R., Case, G. C. R., Chaudry, R. A., James, A. M., Korendyke, C. M., Pike, C. D., Probyn, B. J., Rippington, D. J., Seely, J. F., Tandy, J. A., & Whillock, M. C. R. (2006). Laboratory calibration of the Extreme-ultraviolet Imaging Spectrometer for the Solar-B satellite. Applied Optics, 45(34), 8689–8705. https://doi.org/10.1364/ao.45.008689