Spectral calibration of the atmosphere ultraviolet imaging spectrograph using a PtNe lamp
The atmospheric ultraviolet imaging spectrograph (AUVIS) is an ultraviolet imaging spectrograph that uses a two-dimensional charge-coupled device detector to collect both the spectrum and the swath perpendicular to the flight direction. The design of the system components, the principle, and the main specifications of the AUVIS are introduced. The calibration theory was studied. Considering the characteristics of the AUVIS, a PtNe hollow cathode lamp was chosen as the calibration source, a calibration setup was established, and the AUVIS was calibrated. After the experimental data processing, a function of pixel number-wavelength was established. The uncertainty of the spectral calibration is 0.043 nm.
| Medienart: |
Artikel |
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| Erscheinungsjahr: |
2010 |
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| Erschienen: |
2010 |
| Enthalten in: |
Zur Gesamtaufnahme - volume:30 |
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| Enthalten in: |
Guang pu xue yu guang pu fen xi = Guang pu - 30(2010), 12 vom: 25. Dez., Seite 3302-5 |
| Sprache: |
Chinesisch |
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| Beteiligte Personen: |
Li, Cong [VerfasserIn] |
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| Themen: |
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| Anmerkungen: |
Date Completed 08.07.2015 Date Revised 15.02.2011 published: Print Citation Status PubMed-not-MEDLINE |
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| Förderinstitution / Projekttitel: |
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| PPN (Katalog-ID): |
NLM205874363 |
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| 245 | 1 | 0 | |a Spectral calibration of the atmosphere ultraviolet imaging spectrograph using a PtNe lamp |
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| 500 | |a Date Completed 08.07.2015 | ||
| 500 | |a Date Revised 15.02.2011 | ||
| 500 | |a published: Print | ||
| 500 | |a Citation Status PubMed-not-MEDLINE | ||
| 520 | |a The atmospheric ultraviolet imaging spectrograph (AUVIS) is an ultraviolet imaging spectrograph that uses a two-dimensional charge-coupled device detector to collect both the spectrum and the swath perpendicular to the flight direction. The design of the system components, the principle, and the main specifications of the AUVIS are introduced. The calibration theory was studied. Considering the characteristics of the AUVIS, a PtNe hollow cathode lamp was chosen as the calibration source, a calibration setup was established, and the AUVIS was calibrated. After the experimental data processing, a function of pixel number-wavelength was established. The uncertainty of the spectral calibration is 0.043 nm | ||
| 650 | 4 | |a English Abstract | |
| 650 | 4 | |a Journal Article | |
| 700 | 1 | |a Wang, Yong-Mei |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Guang pu xue yu guang pu fen xi = Guang pu |d 1997 |g 30(2010), 12 vom: 25. Dez., Seite 3302-5 |w (DE-627)NLM09368360X |x 1000-0593 |7 nnns |
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