Solar system: the sun
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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 |
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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 |
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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 |
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Solar
Position Calculations pdf file |
| Solar terrestrial
activity report |
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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 |
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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 |
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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? |
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Sun
colour sun
colour, What colour is the Sun? Blackbody |
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Sunspot Cycle Charts pdf file |
| Sunspots
sunspots are dark areas of irregular shape on the surface of the sun |
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Sunspots
formation of sunspots |
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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 |
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Sunspots and the solar cycle
Sunspots and the solar cycle |
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The path of the sun
in our sky the path of the sun
in our sky |
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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 |
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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 |
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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 |
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The sunspot
cycle |
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Today's Space Weather
Today's Space Weather with black background plots, 3-day Solar-Geophysical
Forecast |
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Ultraviolet wavelengths of the Sun |
| Virtual tour of the sun |
| X-ray
wavelengths the Yohkoh solar observatory satellite |
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Horizontaal |
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Email: support[at]karadimov.info
Last updated on:
2011-01-02
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