Analysis of information sources in references of the Wikipedia article "PGC 2046648" in English language version.
Fig. 1. Cooler Architecture Overview
Fig. 1. Cooler Architecture Overview
The tenuous atmosphere above the 400 km nominal flight altitude has no measurable absorption so that detectors operating at all wavelengths from 5 μm to 1000 μm can achieve high radiometric sensitivity.
Fig. 1. Cooler Architecture Overview
The tenuous atmosphere above the 400 km nominal flight altitude has no measurable absorption so that detectors operating at all wavelengths from 5 μm to 1000 μm can achieve high radiometric sensitivity.
The Observatory is the space-based portion of the James Webb Space Telescope system and is comprisedof three elements: the Integrated Science Instrument Module (ISIM), the Optical Telescope Element (OTE), which includes the mirrors and backplane, and the Spacecraft Element, which includes the spacecraft bus and the sunshield
Fig. 1. Cooler Architecture Overview
The tenuous atmosphere above the 400 km nominal flight altitude has no measurable absorption so that detectors operating at all wavelengths from 5 μm to 1000 μm can achieve high radiometric sensitivity.
Fig. 1. Cooler Architecture Overview
The Observatory is the space-based portion of the James Webb Space Telescope system and is comprisedof three elements: the Integrated Science Instrument Module (ISIM), the Optical Telescope Element (OTE), which includes the mirrors and backplane, and the Spacecraft Element, which includes the spacecraft bus and the sunshield
The tenuous atmosphere above the 400 km nominal flight altitude has no measurable absorption so that detectors operating at all wavelengths from 5 μm to 1000 μm can achieve high radiometric sensitivity.