Simulation and observation of near infrared solar Fe I 1.56 μm line.

Details Simulation and observation of near infrared solar Fe I 1.56 μm line. Simulation and observation of near infrared solar Fe I 1.56 μm line.

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arbei..34...60c&link_type=abstract

Astrophysics Reports, Publications of the Beijing Astronomical Observatory, No. 34, p. 60 - 66

Astronomy and Astrophysics

Astrophysics

Solar Spectrographs: Infrared Lines, Solar Spectrographs: Iron Lines

Scientific paper

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.

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