3. Natural Climate Variability. SPM 1b Variations of the Earth’s surface temperature for the past 1,000 years Approx. climate range over the 900 years.
Chapter 21 Review Place these notes into your Meteorology Notebook.
It can be powered by NUCLEAR ENERGY! Luminosity ~ 10 billion years Nuclear Potential Energy (core) E = mc 2 - Einstein, 1905.
The Solar Cycle for seeing the sun exhibit. The Sun’s Magnetic Field The magnetic field on the sun is produced by the flow of electrically charged ions.
Solar rotation and activity from Galileo to the present Dr. David Pundak 1 and Dr. Lev Pustilnik 2 1 Kinneret Academic College,Jordan Valley, Israel 2.
N.V. Semenova Polar Geophysical Institute, Apatity, Russia.
We continue to learn a lot about the solar system by using space exploration.
Greenhouse Effect The greenhouse effect is a process by which thermal radiation from a planetary surface is absorbed by atmospheric green house gases,
+ The Sun. Sun Facts Makes life on our planet possible by giving us great amounts of light and heat Contains about 98% of the mass of the entire Solar.
Solar Rotation Lab 3. Differential Rotation The sun lacks a fixed rotation rate Since it is composed of a gaseous plasma, the rate of rotation is fastest.
The Dangers of Solar Storms and Solar Cycles. For every 1 million atoms of hydrogen in the entire sun 98,000 atoms of helium 850 of oxygen 360.
EARTH & SPACE SCIENCE Chapter 29 The Sun 29.2 Solar Activity.
