Jump to content

Solar flux unit

From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by Citation bot (talk | contribs) at 04:51, 7 November 2021 (Removed proxy/dead URL that duplicated identifier. | Use this bot. Report bugs. | Suggested by Abductive | #UCB_toolbar). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

The solar flux unit (sfu) is a convenient measure of spectral flux density often used in solar radio observations, such as the F10.7 solar activity index:[1]

1 sfu = 104 Jy = 10−22 W⋅m−2⋅Hz−1 = 10−19 erg⋅s−1⋅cm−2⋅Hz−1.

See jansky for further information about related units.

References

  1. ^ Tapping, K. F. (2013). "The 10.7 cm solar radio flux (F10.7)". Space Weather. 11 (7): 394–406. Bibcode:2013SpWea..11..394T. doi:10.1002/swe.20064.