Paper
1 October 1993 Cosmic background explorer (COBE) mission
Author Affiliations +
Abstract
The Cosmic Background Explorer (COBE) satellite carries three instruments to measure the diffuse infrared and microwave background radiation from the early universe, along with more recent diffuse sources. It was developed by NASA's Goddard Space Flight Center and launched by a Delta rocket on November 18, 1989. It has produced the first measurements of structure in the Big Bang and has shown that the primeval heat radiation has a blackbody spectrum to extraordinary accuracy. The three instruments include a Far Infrared Absolute Spectrophotometer (FIRAS) to cover the range from 100 micrometers to 1 cm wavelength with a 7 degree(s) resolution, a Diffuse Infrared Background Experiment (DIRBE) to map the sky from 1 to 300 micrometers with a 0.7 degree(s) resolution in 10 broad bands, and a Differential Microwave Radiometer (DMR) to map the sky at 31.5, 53, and 90 GHz with a 7 degree(s) resolution. The designs of the instruments and spacecraft are described, and the primary results ar summarized.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
John C. Mather "Cosmic background explorer (COBE) mission", Proc. SPIE 2019, Infrared Spaceborne Remote Sensing, (1 October 1993); https://doi.org/10.1117/12.157821
Lens.org Logo
CITATIONS
Cited by 13 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Space operations

Calibration

Infrared radiation

Sun

Helium

Radiometry

Sensors

RELATED CONTENT

In orbit performance of the AVHRR, HIRS, and AMSU A...
Proceedings of SPIE (September 19 2013)
Evaluating uniformity of IR reference sources
Proceedings of SPIE (October 13 2015)
The evolution of the performance of the AVHRR, HIRS and...
Proceedings of SPIE (October 24 2012)
The evolution of the performance of the AVHRR, HIRS and...
Proceedings of SPIE (September 16 2011)

Back to Top