The detection of various cryogenic targets, including the polar cryosphere,
high-altitude clouds, and cosmic galaxies through spectral analysis,
is a highly valuable area of research. Nevertheless, creating a very
long wave infrared (VLWIR) imaging spectrometer capable of detecting
these targets presents a significant challenge. In this paper, we
introduce a design concept for an ultra-wide temperature difference
athermalization VLWIR multifunctional imaging spectrometer. Initially,
we analyze the multifunctional characteristics of an imaging
spectrometer that utilizes a coaxial optical layout. Subsequently, we
delve into the constraints associated with smile aberration correction
and coaxial optical layout of the imaging spectrometer, which utilizes
a grism as the dispersion component. Finally, we construct a
computational model to determine the parameters of the grism. In the
study, we provide evidence that imaging spectrometers with symmetrical
structural forms can effectively minimize the impact of temperature
variations on the system. Building on these findings, we developed the
ultra-wide temperature difference athermalization VLWIR
multifunctional imaging spectrometer, which boasts a temperature
variation range over 200 K. This versatile instrument features
a multifunctional mode that can be easily tuned to meet a range of
observation missions. The spectrometer has a spectral range of 12µm to 16µm, a field of view (FoV) of 16.8mm×6mm, a numerical aperture (NA) of 0.334,
an alignment temperature of 293.15 K, and an operating
temperature of 60 K. The analysis results demonstrate the many
working modes and high imaging quality of the designed imaging
spectrometer. This paper’s research offers a fresh approach for
low-temperature VLWIR imaging spectrometer systems.