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Twenty years later the Spitzer Space Telescope, with greater sensitivity, greater wavelength coverage, and better resolution, mapped many dust complexes in the Milky Way.
The wavelength coverage and tunability mechanisms are also discussed.
Hence, wavelength coverage is crucial in our study.
The wavelength coverage and views of the planet also differ for all three missions.
The SUMER instrument has a very broad wavelength coverage, from roughly 660 to 1610 Å.
ASTRO-F is a perfect complement to Spitzer Space Telescope in respect of its wide sky and wavelength coverage.
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A round robin test for GLI (Global Imager) instrument was conducted with the three transfer spectrometers, 400 800 nm, 500 1000 nm and 1300 2500 nm of the wavelength coverages, respectively.
In particular, they should have good single photon sensitivity for visible and UV wavelengths and large coverage with fine granularity.
These promising improvements can be attributed to three important factors of the ZnO/CdSe core/shell nanoneedle-based solar cell: strong light absorption in a wider wavelength range; higher CdSe coverage on ZnO surface, and direct contact between CdSe and ZnO without any interlinking material.
We have developed CD and LD measuring technique by polarization modulation at the source, without using transmission type polarizing modulator, to extend to the coverage to wavelengths shorter than 140 nm.
Since the 1990s, the ranges of wavelengths available, swath coverages and repeat measurement intervals have increased (Table 1).
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