Astrophysics (Index)About

bolometer

(instrument measuring heat produced by radiation)

A bolometer is a type of instrument that measures electromagnetic radiation (EMR) by allowing the radiation to heat a metal whose electrical resistance is dependent upon its temperature. As the material heats, the change in resistance is measured. Bolometers measure a relatively wide range of EMR frequencies, thus are more suited to measuring energy over a wide range or estimating the total incident energy from a source, but they are not necessarily the most sensitive instruments for some frequency ranges. They can be made competitive in the submillimeter to 1 mm range (far infrared). To achieve sensitivity, such bolometers are cooled to near absolute zero. Micro-bolometers laid out in grid arrays are used for imaging, with on the order of 100 × 100 pixels, and more recently approaching 1000 × 1000.

Note that the adjective bolometric which has the obvious meaning "involving bolometers", is also very often used to indicate the total of all EMR, for example, all that from a particular source. This is the intended meaning in terms like bolometric correction, bolometric luminosity, and bolometric magnitude. This presumably came about because bolometers do indeed measure the power of the EMR striking it across a wide band wider than many other instruments, though they are not complete in that regard, and also, an Earth-bound bolometer will necessarily miss radiation not within atmospheric windows.


(instrument type,EMR,submillimeter)
Further reading:
https://en.wikipedia.org/wiki/Bolometer
https://en.wikipedia.org/wiki/Microbolometer
https://glossary.ametsoc.org/wiki/Bolometer
https://www.britannica.com/technology/bolometer
https://www.chemeurope.com/en/encyclopedia/Bolometer.html
https://stratocat.com.ar/stratopedia/232.htm
http://www.submm.caltech.edu/kids_html/DM/SiN_papers/benford_2003.pdf

Referenced by pages:
ACBAR
Atacama Cosmology Telescope (ACT)
Atacama Pathfinder Experiment (APEX)
Atacama Submillimeter Telescope Experiment (ASTE)
AzTEC-3
bolometric luminosity (LBol)
BOOMERanG
CMB Stage-4 (CMB-S4)
EBEX
focal plane array (FPA)
front end instrument
GISMO
Green Bank Telescope (GBT)
IRAM 30m Telescope
James Clerk Maxwell Telescope (JCMT)
JINGLE
KID
LSPE-SWIPE
MAXIMA
microcalorimeter
MUSTANG
QUaD
QUBIC
radiometer
SCUBA
SOFIA
South Pole Telescope (SPT)
SQUID
superconducting tunnel junction (STJ)
Swedish-ESO Submillimetre Telescope (SEST)
transition edge sensor (TES)

Index