Jansky

jansky
Unit systemNon-SI metric unit
Unit ofFlux density
SymbolJy
Named afterKarl Guthe Jansky
Conversions
1 Jy in ...... is equal to ...
   SI units   10−26 W⋅m−2⋅Hz−1
   CGS units   10−23 erg⋅s−1⋅cm−2⋅Hz−1

The jansky (symbol Jy, plural janskys) is a non-SI unit of spectral flux density,[1] or spectral irradiance, used especially in radio astronomy. It is equivalent to 10−26 watts per square metre per hertz.

The flux density or monochromatic flux, S, of a source is the integral of the spectral radiance, B, over the source solid angle:

The unit is named after pioneering US radio astronomer Karl Guthe Jansky and is defined as

  • (SI)[2]
  • (cgs).

Since the jansky is obtained by integrating over the whole source solid angle, it is most simply used to describe point sources; for example, the Third Cambridge Catalogue of Radio Sources (3C) reports results in janskys.

  • For extended sources, the surface brightness is often described with units of janskys per solid angle; for example, far-infrared (FIR) maps from the IRAS satellite are in megajanskys per steradian (MJy⋅sr−1).
  • Although extended sources at all wavelengths can be reported with these units, for radio-frequency maps, extended sources have traditionally been described in terms of a brightness temperature; for example the Haslam et al. 408 MHz all-sky continuum survey is reported in terms of a brightness temperature in kelvin.[3]
  1. ^ "International Astronomical Union | IAU". www.iau.org.
  2. ^ Burke, Bernard F.; Graham-Smith, Francis (2009). An Introduction to Radio Astronomy (3rd ed.). Cambridge University Press. p. 9. ISBN 978-0-521-87808-1.
  3. ^ Haslam, C. G. T. (1 March 1985). "The 408 MHz all-sky continuum survey". Bulletin d'Information du Centre de Donnees Stellaires. 28: 49. Bibcode:1985BICDS..28...49H. ISSN 1169-8837.