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فائل:Thermohaline Circulation 2.png

صفحي جو مواد ٻين ٻولين ۾ سپورٽ نہ ڪيو ويو آھي.
کليل ڄاڻ چيڪلي، وڪيپيڊيا مان

اصلوڪو فائيل(1,100 × 690 عڪسلون، فائيل سائيز: 122 KB، MIME ٽائيپ: image/png)

ھي فائيل وڪيميڊيا العام مان آھي ۽ ٻين رٿائن پاران پڻ استعمال ٿي سگهي ٿو. تشريح انجي [فائيل جي تشريحي صفحي] ھيٺان ڏنل آھي.

تَتُ

تشريح
English: This map shows the pattern of thermohaline circulation also known as "meridional overturning circulation". This collection of currents is responsible for the large-scale exchange of water masses in the ocean, including providing oxygen to the deep ocean. The entire circulation pattern takes ~2000 years.
Deutsch: Thermohaline Zirkulation und die Entstehung von kaltem, dichtem Tiefenwasser im Nordmeer
تاريخ
ذريعو NASA Earth Observatory
ليکڪ Robert Simmon, NASA. Minor modifications by Robert A. Rohde also released to the public domain
اجازت
(ھن فائيل کي وَراستعمال ڪندي)
Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
Warnings:
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عنوان

ھڪ-سٽي وضاحت ڏيو تہ ھي فائيل ڇاکي ٿو ظاھر ڪري

Items portrayed in this file

depicts انگريزي

inception انگريزي

29 مارچ 2008

فائيل جي سوانح

ڪنھن بہ تاريخ/وقت تي ٽڙڪ ڪري ڏسندا تہ ان وقت اهو فائيل ڪيئن هو.

تاريخ/وقتآڱوٺي ننھنماپَواپرائيندڙراءِ
موجود نسخو20:08, 29 مارچ 200820:08, 29 مارچ 2008 جي نظرثاني لاءِ تصويري نشان1,100 × 690 (122 KB)Dragons flight{{Information |Description=This map shows the pattern of w:thermohaline circulation also known as "meridional overturning circulation". This collection of currents is responsible for the large-scale exchange of water masses in the ocean, including p

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