You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
Infrared radiometers and spectrometers generally use blackbodies for calibration, and with the high accuracy needs of
upcoming missions, blackbodies capable of meeting strict accuracy requirements are needed. One such mission, the
NASA climate science mission Climate Absolute Radiance and Refractivity Observatory (CLARREO), which will
measure Earth's emitted spectral radiance from orbit, has an absolute accuracy requirement of 0.1 K (3σ) at 220 K over
most of the thermal infrared. Space Dynamics Laboratory (SDL) has a blackbody design capable of meeting strict
modern accuracy requirements. This design is relatively simple to build, was developed for use on the ground or onorbit,
and is readily scalable for aperture size and required performance. These-high accuracy blackbodies are currently
in use as a ground calibration unit and with a high-altitude balloon instrument. SDL is currently building a prototype
blackbody to demonstrate the ability to achieve very high accuracy, and we expect it to have emissivity of ~0.9999 from
1.5 to 50 μm, temperature uncertainties of ~25 mK, and radiance uncertainties of ~10 mK due to temperature gradients.
The high emissivity and low thermal gradient uncertainties are achieved through cavity design, while the low
temperature uncertainty is attained by including phase change materials such as mercury, gallium, and water in the
blackbody. Blackbody temperature sensors are calibrated at the melt points of these materials, which are determined by
heating through their melt point. This allows absolute temperature calibration traceable to the SI temperature scale.
The alert did not successfully save. Please try again later.
Harri M. Latvakoski, Mike Watson, Shane Topham, Deron Scott, Mike Wojcik, Gail Bingham, "Accurate blackbodies," Proc. SPIE 7739, Modern Technologies in Space- and Ground-based Telescopes and Instrumentation, 773919 (19 July 2010); https://doi.org/10.1117/12.857171