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gallery - hot solar atmosphere

 

Gallery - Hot solar atmosphere

 
Sun|trek movies are now available on our YouTube Channel
 

TRACE movie of ultraviolet loops in the Sun's atmosphere. The hot, million degree plasma traces out the magnetic field. Waves can propagate along these loops.[Movie file 1mb or more - High quality]

 

 

TRACE movie of ultraviolet loops in the Sun's atmosphere. The hot, million degree plasma traces out the magnetic field. Waves can propagate along these loops.

 

TRACE ultraviolet movie of an active region. Waves can be seen to move through the atmosphere along the loops. The movement of the wave's energy to the surrounding plasma is one way that the corona could be heated.[Movie file 1mb or more - High quality]

 

 

TRACE ultraviolet movie of an active region. Waves can be seen to move through the atmosphere along the loops. The movement of the wave's energy to the surrounding plasma is one way that the corona could be heated.

 

Movie of the 1994 total solar eclipse. The Moon can be seen to move in front of the Sun. When the total eclipse is occurring, the solar atmosphere (corona) can be seen around the limb of the Moon.[Movie file 1mb or more - High quality]

 

 

Movie of the 1994 total solar eclipse. The Moon can be seen to move in front of the Sun. When the total eclipse is occurring, the solar atmosphere (corona) can be seen around the limb of the Moon.

 

Movie showing the path of the eclipse shadow across the Earth. The eclipse shown in the movie could be viewed from the pacific ocean and central and south America .[Movie file 1mb or more - High quality]

 

 

Movie showing the path of the eclipse shadow across the Earth. The eclipse shown in the movie could be viewed from the pacific ocean and central and south America .

 

Movie of a full-Sun magnetic field simulation, which is based on the magnetic field measurements at the surface of the Sun. There are closed magnetic field structures, which link sunspots together. There are also open magnetic field structures, which stretch out into space.[Movie file 1mb or more - High quality]

 

 

Movie of a full-Sun magnetic field simulation, which is based on the magnetic field measurements at the surface of the Sun. There are closed magnetic field structures, which link sunspots together. There are also open magnetic field structures, which stretch out into space.

 

Movie of an emerging magnetic field simulation. The temperature of the solar atmosphere increases at the top of the newly emerged magnetic field. It then interacts with the existing magnetic field in the atmosphere.[Movie file 1mb or more - High quality]

 

 

Movie of an emerging magnetic field simulation. The temperature of the solar atmosphere increases at the top of the newly emerged magnetic field. It then interacts with the existing magnetic field in the atmosphere.

 

Movie of a simulation of the magnetic field in a sunspot. The magnetic field in the sunspot is anchored deep in the solar interior. The magnetic field in the solar atmosphere above the sunspot is very dynamic and is buffeted around by the motions at the surface and in the atmosphere.[Movie file 1mb or more - High quality]

 

 

Movie of a simulation of the magnetic field in a sunspot. The magnetic field in the sunspot is anchored deep in the solar interior. The magnetic field in the solar atmosphere above the sunspot is very dynamic and is buffeted around by the motions at the surface and in the atmosphere.

 

Movie of a sunspot in visible light and a simulation of the structure of the sunspot. In the simulation the red areas are hot and the blue areas are cool. The simulation also shows the convective patterns, which transport energy from inside the Sun to the surface.[Movie file 1mb or more - High quality]

 

 

Movie of a sunspot in visible light and a simulation of the structure of the sunspot. In the simulation the red areas are hot and the blue areas are cool. The simulation also shows the convective patterns, which transport energy from inside the Sun to the surface.

 

Movie of a convection simulation. This shows how the energy in the convection zone is transported to the surface of the Sun.[Movie file 1mb or more - High quality]

 

 

Movie of a convection simulation. This shows how the energy in the convection zone is transported to the surface of the Sun.

 

Still Images

Baily beads CDS EIT Loop systems Corona during an eclipse Corona spectral lines Creasent sun
Dimond ring electromagnetic radiation fraunhofer spectrum Fred Espenak eclipse Hot corona
Dragon Prism Shibata emerging flux SOHO EIT helium Spectra emmision
Steiner sunspot magnetic flux Sunspot flow Wave Wegalmann magnetic Sun  

 

 

Take a look around the rest of the Sun|trek gallery for more pictures and movies of the Sun, our star, used in Sun|trek. To make it simpler we have arranged everything according to where they feature within the Sun|trek adventure sections.

 
[Gallery - Solar surface & below] [Gallery - Hot solar atmosphere] [Gallery - Magnetic Sun] [Gallery - Flowing from the Sun]
[Gallery - Sun-Earth connection] [Gallery - Solar spacecraft] [Gallery - Earth & beyond] [Gallery - The Sun as a Star]
 

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