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Horizontaal
Solar system: the sun
3-D Images of the Sun NASA's Solar TErrestrial RElations Observatory (STEREO) satellites have provided the first three-dimensional images of the sun. For the first time, scientists will be able to see structures in the sun's atmosphere in three dimensions. The new view will greatly aid scientists' ability to understand solar physics and there by improve space weather forecasting. This web page contains 3-D anaglyph video and images. This 3-D video can be seen with red and cyan + 3-D paper glasses
Current solar images
Solar center a collection of fun educational activities based on solar oscillations investigation, the sun's tangled magnetic field
Solar Dynamics Observatory
Solar flux Solar Terrestrial Activity Report
Solar max 2000 links and information about solar cycle
Solar on line activity resources a collection of fun educational activities based on solar oscillations investigation
Solar Position Calculations pdf file
Solar terrestrial activity report
Stanford solar center this site presents a collection of fun educational activities where educators and students can explore the Sun's tangled magnetic field, its turbulent surface motions, the dramatic sunspot cycle, and even what magic happens in the solar interior where instrumental eyes cannot penetrate
Sun as a star Solar Properties, The Sun Compared with Other Stars, What is The Structure of the Sun, Cross Section of the Sun, The chromosphere, The Solar Corona, Solar flares, Coronal Mass Ejections, The Solar Magnetic Field, Solar Phenomena on Other Stars
Sunbeams sunbeams, What is our Sun anyway? What color is Sunlight? What's our Sun like on the inside? What's the strangest thing about our Sun? Does our Sun spin like Earth does? Does our Sun always look the same?
Sun colour sun colour, What colour is the Sun? Blackbody
Sunspot Cycle Charts pdf file
Sunspots sunspots are dark areas of irregular shape on the surface of the sun
Sunspots formation of sunspots
Sunspots formation of sunspots, Sunspots are observed to start forming at latitude 30oN and 30oS of the Sun's Equator. The regions in which sunspots are formed are known as active regions. The formation of sunspots is due to the differential rotation of the Sun. Differential rotation is a phenomenon whereby different parts of the Sun rotates at different speed
Sunspots and the solar cycle every 11 years the sun undergoes a period of activity called the "solar maximum", followed by a period of quiet called the "solar minimum". During the solar maximum there are many sunspots, solar flares, and coronal mass ejections, Educypedia
Sunspots and the solar cycle Sunspots and the solar cycle
The path of the sun in our sky the path of the sun in our sky
The Sun Sunlight and the Earth, Weather and the Atmosphere, Global Climate, Global Wind flow, Our View of the Sun, The Magnetic Sun, Interplanetary Magnetic Field Lines, The Many Colors of Sunlight, Experimenting with Colors, Waves and Photons, Quantum Physics, The Atomic Structure of Matter, Atomic Energy Levels, Planck's Constant: Radiation from Hot Objects, The Atomic Nucleus and Bohr's Early Model of the Atom, Expansion of the Bohr Model, Wave Mechanics, Quantum Tunneling
The Sun The Sun images
The sun a pictorial introduction nearly 1392000 km in diameter and 1.989 x 1030 kg in mass, the sun is the geometric and gravitational center of the planetary system
The sunspot cycle Sunspot Numbers, The Maunder Minimum, The Butterfly Diagram, The Greenwich Sunspot Data, Sunspot Cycle Predictions, The Interior, The Photosphere, The Chromosphere, The Transition Region, The Corona, The Solar Wind, The Heliosphere
The sunspot cycle
Today's Space Weather Today's Space Weather with black background plots, 3-day Solar-Geophysical Forecast
Ultraviolet wavelengths of the Sun
Virtual tour of the sun
X-ray wavelengths the Yohkoh solar observatory satellite
Horizontaal

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Last updated on: 2011-01-02 | Copyright © 2011-2013 Educypedia.

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