Tangent arcs: Difference between revisions

From Glossary of Meteorology
imported>Perlwikibot
(Created page with " {{TermHeader}} {{TermSearch}} <div class="termentry"> <div class="term"> == tangent arcs == </div> <div class="definition"><div class="short_definition">A halo in ...")
 
imported>Perlwikibot
No edit summary
 
(One intermediate revision by the same user not shown)
Line 9: Line 9:
   </div>
   </div>


<div class="definition"><div class="short_definition">A [[halo]] in the form of an arc tangent to a circular halo.</div><br/> <div class="paragraph">The most common of these are the upper and lower tangent arcs to the [[halo of 22&deg;]]. They form  separate arcs when the sun is low, but as the sun climbs they join to produce the [[circumscribed  halo]]. These arcs are explained by [[refraction]] through the 60&deg; prism sides of columnar crystals  oriented with their long axes horizontal. <br/>''See'' [[46&deg; lateral arcs]].</div><br/> </div>
<div class="definition"><div class="short_definition">A [[halo]] in the form of an arc tangent to a circular halo.</div><br/> <div class="paragraph">The most common of these are the upper and lower tangent arcs to the [[halo|halo of 22&#x000b0;]]. They form  separate arcs when the sun is low, but as the sun climbs they join to produce the [[circumscribed halo|circumscribed  halo]]. These arcs are explained by [[refraction]] through the 60&#x000b0; prism sides of columnar crystals  oriented with their long axes horizontal. <br/>''See'' [[46&#x000b0; lateral arcs]].</div><br/> </div>
</div>
</div>



Latest revision as of 17:03, 25 April 2012



tangent arcs

A halo in the form of an arc tangent to a circular halo.

The most common of these are the upper and lower tangent arcs to the halo of 22°. They form separate arcs when the sun is low, but as the sun climbs they join to produce the circumscribed halo. These arcs are explained by refraction through the 60° prism sides of columnar crystals oriented with their long axes horizontal.
See 46° lateral arcs.


Copyright 2024 American Meteorological Society (AMS). For permission to reuse any portion of this work, please contact permissions@ametsoc.org. Any use of material in this work that is determined to be “fair use” under Section 107 of the U.S. Copyright Act (17 U.S. Code § 107) or that satisfies the conditions specified in Section 108 of the U.S.Copyright Act (17 USC § 108) does not require AMS’s permission. Republication, systematic reproduction, posting in electronic form, such as on a website or in a searchable database, or other uses of this material, except as exempted by the above statement, require written permission or a license from AMS. Additional details are provided in the AMS Copyright Policy statement.