Infrared Instrumentation Sample Clauses

Infrared Instrumentation. The XxXxxx-Xxxxxx facility is the world’s only large solar telescope without an entrance window, thus giving it unique access to the solar infrared spectrum beyond 2.5 microns. NSO has focused its in-house instrumentation program on a large format IR camera, the NSO Array Camera (NAC), which will observe wavelengths from 1 to 5 microns. NAC is being built using an ALADDIN-III InSb array with electronics and a cryostat from Mauna Kea Infrared (MKIR). With 16 times as many pixels, higher quantum efficiency, and lower read-out noise, the NAC represents a significant improvement over previous NSO IR cameras. New types of scientific observations will be enabled by the NAC at the XxXxxx-Xxxxxx, such as sensitive magnetic field measurements in sunspot umbra, studies of molecular line formation, and opportunities for polarimetric observations from 3 to 5 microns. The NAC will also open new windows on flares and other solar processes (like Evershed flows) at infrared wavelengths. In addition to these PI- driven studies, NSO is exploring using the NAC for regular highly sensitive vector magnetograms of solar active regions in synoptic or campaign-mode observing runs. Implementing and demonstrating the scientific value of a fast, large-format infrared camera is an important component of NSO's preparation for the IR-capable ATST. The initial operation of a large- format, advanced IR instrument at the XxXxxx-Xxxxxx solar telescope facility will offer the most advanced research capability in the mid-IR for solar physics in the world today.
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