Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
NRLMSISE-00
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
[[Image:Atmosphere model.png|thumb|right|280px|NRLMSISE output]] '''NRLMSISE-00''' is an [[empirical]], global [[reference atmospheric model]] of the Earth from ground to space.<ref>{{Cite journal|last1=Picone|first1=J. M.|last2=Hedin|first2=A. E.|last3=Drob|first3=D. P.|last4=Aikin|first4=A. C.|date=2002-12-01|title=NRLMSISE-00 empirical model of the atmosphere: Statistical comparisons and scientific issues|journal=Journal of Geophysical Research: Space Physics|language=en|volume=107|issue=A12|pages=1468|doi=10.1029/2002JA009430|issn=2156-2202|bibcode=2002JGRA..107.1468P|hdl=2060/20020038771|hdl-access=free}}</ref> It models the [[temperature]]s and [[density|densities]] of the atmosphere's components. A primary use of this model is to aid predictions of [[satellite]] orbital decay due to [[atmospheric drag]]. This model has also been used by astronomers to calculate the mass of air between telescopes and laser beams in order to assess the impact of [[laser guide stars]] on the non-lasing telescopes.<ref>Coulson, Dolores M. & Roth, Katherine C., Adaptive Optics Systems II. Edited by Ellerbroek, Brent L.; Hart, Michael; Hubin, Norbert; Wizinowich, Peter L. Proceedings of the SPIE, Volume 7736, pp. 773652-773652-9 (2010)</ref>
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)