Methods for rejecting daytime waste heat to outer space
Abstract
We report that outer space constitutes an extremely low temperature (T ~ 4 K) thermodynamic reservoir of boundless thermal capacity, with the potential to serve as a cold reservoir for cooling objects to sub-ambient temperatures in the daytime. For example, assuming a perfect emitter at 300 K, the theoretical black-body heat transfer rate to space can be calculated to be 450 Wm-2 [1]. However, for terrestrial objects, the atmosphere serves as a highly effective infrared (IR) insulator, as well as a heat source via radiation, convection and conduction to the object when cooled to sub-ambient temperatures.
- Authors:
-
- USDOE Advanced Research Projects Agency - Energy (ARPA-E) (United States)
- Publication Date:
- Research Org.:
- USDOE Advanced Research Projects Agency - Energy (ARPA-E), Washington, DC (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1464730
- Resource Type:
- Accepted Manuscript
- Journal Name:
- National Science Review
- Additional Journal Information:
- Journal Volume: 4; Journal Issue: 6; Journal ID: ISSN 2095-5138
- Publisher:
- China Science Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 54 ENVIRONMENTAL SCIENCES
Citation Formats
Stark, Addison K. Methods for rejecting daytime waste heat to outer space. United States: N. p., 2017.
Web. doi:10.1093/nsr/nwx052.
Stark, Addison K. Methods for rejecting daytime waste heat to outer space. United States. https://doi.org/10.1093/nsr/nwx052
Stark, Addison K. Tue .
"Methods for rejecting daytime waste heat to outer space". United States. https://doi.org/10.1093/nsr/nwx052. https://www.osti.gov/servlets/purl/1464730.
@article{osti_1464730,
title = {Methods for rejecting daytime waste heat to outer space},
author = {Stark, Addison K.},
abstractNote = {We report that outer space constitutes an extremely low temperature (T ~ 4 K) thermodynamic reservoir of boundless thermal capacity, with the potential to serve as a cold reservoir for cooling objects to sub-ambient temperatures in the daytime. For example, assuming a perfect emitter at 300 K, the theoretical black-body heat transfer rate to space can be calculated to be 450 Wm-2 [1]. However, for terrestrial objects, the atmosphere serves as a highly effective infrared (IR) insulator, as well as a heat source via radiation, convection and conduction to the object when cooled to sub-ambient temperatures.},
doi = {10.1093/nsr/nwx052},
journal = {National Science Review},
number = 6,
volume = 4,
place = {United States},
year = {Tue May 02 00:00:00 EDT 2017},
month = {Tue May 02 00:00:00 EDT 2017}
}
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Cited by: 4 works
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Figures / Tables:
Fig. 1: (A) The spectral power density of the incident solar irradiance and blackbody radiation from a room temperature emitter are plotted. Due to the order of magnitude difference, a highly effective selective emitter is required to simultaneously reflect the solar irradiance while still emitting within the 8-13μm sky-window. (B)more »
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Works referenced in this record:
Ultrabroadband Photonic Structures To Achieve High-Performance Daytime Radiative Cooling
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Works referencing / citing this record:
Radiative sky cooling: Fundamental principles, materials, and applications
journal, June 2019
- Zhao, Dongliang; Aili, Ablimit; Zhai, Yao
- Applied Physics Reviews, Vol. 6, Issue 2
Figures/Tables have been extracted from DOE-funded journal article accepted manuscripts.