Simulation and observation of near infrared solar Fe I 1.56 μm line.
Abstract
The infrared focal plane array (IRFPA) with large size and high quantum efficiency is very difficult to acquire. On Jan. 29 - 30, 1999, the authors utilized PtSi IRFPA to observe the infrared solar Fe I 1.56 μm line. The simulation and observation for this experiment are introduced in detail.
- Publication:
-
Astrophysics Reports Publications of the Beijing Astronomical Observatory
- Pub Date:
- December 1999
- Bibcode:
- 1999ArBei..34...60C
- Keywords:
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- Solar Spectrographs: Infrared Lines;
- Solar Spectrographs: Iron Lines