In July and August, the ITCZ lies well to <u>the</u><u> north of the equator </u><u>over Africa, Asia and Central America before going to south</u> into South America, central Africa and Australia by January and February.
<u>In January the </u><u>ITCZ</u><u> lies about at 15°S over</u><u> South America and Africa.</u><u> The</u><u> ITCZ</u><u> is less mobile over the oceans,</u> where it binds a stationary position just north of the equator.
<h3>What is the ITCZ ?</h3>
The Intertropical Convergence Zone, or ITCZ, is defined as a band of low pressure around the Earth which commonly lies near to the equator. The trade winds of the northern and southern hemispheres meet here, which takes them to the development of frequent thunderstorms and heavy rain.
<h3>What is the characteristics of ITCZ?</h3>
The ITCZ is characterized by low atmospheric pressures, as a result of the upward movement induced by the trade winds convergence. It forms a high atmospheric pressure in the upper troposphere.
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First off you should really type the equation in the proper order and also use the carat symbol to show that something is to the power too, so your equation shouldve looked like this.
-y^2 -4y + 4 = 0
But all yuo need to is plug the equation into a calculator and search for where it intersects the X line. the answers are
(.828, 0) , (-4.83, 0)
Answer:
Hukbo ng Bayan Laban sa Hapon
Explanation:
The Hukbalahap (short for Hukbo ng Bayan Laban sa Hapon, or National Armed Force against the Japanese) started as a resistance movement against the Japanese occupiers
Answer:
Weathering
Explanation:
Weathering because erosion is water or air hollowing or degrading rock.
Answer:
The interior of Mars is probably solid.
Explanation:
The Earth's magnetic dynamo is generated by a current in the interior of the planet that is a result of the eddies that form thanks to the outer core being molten.
Since Mars is a smaller planet and is located twice as far from the Sun as Earth, it cooled faster and likely no longer has a molten or semi-molten interior. The cooling of the interior of the planet would have shut off the magnetic process and could explain why the modern Martian atmosphere is so tenuous.
