Vertical motions in the Uranian atmosphere: an analysis of radio observations

Clicks: 9
ID: 268047
1990
Free PDF
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This article has not been analysed, so there is no overall score — reader engagement is measured and shown alongside.
AI Quality Assessment
Not analyzed
Readership in this journal
Star

Ranked #12 of 12 articles by views in icarus

Most read Least read

Bar heights use a square-root scale.

Mint this article as an NFT
Not yet minted

Create a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.

5 SUSD one-off · no wallet required
Sign in to mint
Abstract
We present a new 6-cm radio map of Uranus that shows latitudinal features probably caused by vertical motions in the atmosphere. A comparison with older data and Voyager infrared measurements suggests that large-scale vertical motions have not changed significantly in the last 8 years, and that these motions are deep seated and extend from the 0.1- to the 45-bar level—a height of 250 km.
Reference Key
muhleman1990icarusvertical Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Mark D. Hofstadter,Glenn L. Berge,Duane O. Muhleman;Mark D. Hofstadter;Glenn L. Berge;Duane O. Muhleman;
Journal icarus
Year 1990
DOI
10.1016/0019-1035(90)90170-e
URL
https://sciprofiles.com/publication/view/378c93ac5a2230b4ba0352cecf668878
Keywords
vertical motions uranian atmosphere radio observations radio map cm radio bar level

Citations

No citations found. To add a citation, contact the admin at info@scimatic.org

Comments

No comments yet. Be the first to comment on this article.