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Climatology, Chapter 3

by: Rose Notetaker

Climatology, Chapter 3 ES 385

Rose Notetaker
GPA 3.0

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About this Document

Dr. Anthony Vega
Class Notes
Climatology, chapter 3, Vega
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This 1 page Class Notes was uploaded by Rose Notetaker on Tuesday February 9, 2016. The Class Notes belongs to ES 385 at Clarion University of Pennsylvania taught by Dr. Anthony Vega in Spring 2016. Since its upload, it has received 20 views. For similar materials see Climatology in Earth Sciences at Clarion University of Pennsylvania.

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Date Created: 02/09/16
Latitude Latitude- imaginary lines that run from west to east around the Earth, parallel to the equator and each other - Equator = 0 degrees - North and South Poles= 90 degrees - Indicate the location of a place relative to the equator Longitude- imaginary north-south lines running through the North and South Poles perpendicular to the equator - Aka meridians , are not parallel to each other they converge toward the poles - Measures the angle created between the point of interest Prime Meridian- runs through Greenwich, England, which is at 0 degrees longitude *As latitude increases solar energy (radiation), strike the surface at decreasing angles depending on where the sun is located Attenuation- depletion of solar rays Earth-Sun Relationships Revolution- orbit around the Sun - The path is not completely circular around the Sun it is elliptical Rotation- spin of the Earth on its axis, the earth spins west to east (counterclockwise) when view from above the North Pole - One rotation occurs every 24 hours or 15 degrees every hour - Causes divisions of time zones Plane of the Ecliptic- represents the plane that bisects both Earth and Sun Axis Tilt- Fixed at 23.5 degrees - This principle is known as parallelism


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