Jump to content

Solar flux unit

Edit links
From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by Citation bot (talk | contribs) at 01:51, 8 January 2021 (Add: bibcode, pages, issue, volume, journal, year, title, doi, author pars. 1-1. Converted bare reference to cite template. Formatted dashes. | You can use this bot yourself. Report bugs here. | Suggested by Abductive | Category:Astronomy stubs‎ | via #UCB_Category 37/391). 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.


Stub icon

This standards- or measurement-related article is a stub. You can help Wikipedia by expanding it.

Stub icon

This astronomy-related article is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=Solar_flux_unit&oldid=999007456"