Changes between Version 9 and Version 10 of AstroBearGallery


Ignore:
Timestamp:
06/01/11 19:16:18 (14 years ago)
Author:
Erica Kaminski
Comment:

Legend:

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  • AstroBearGallery

    v9 v10  
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    12 '''''Magnetic field lines oriented in the x-direction and their interaction with a hypersonic clumpy flow.''''' A Mach-25 speed wind is continuously injected into the grid from the left where it encounters and disperses a field of denser rings of gas clumps. The dynamic interplay between the clumps, shocks, and magnetic field is illustrated in these synthetic schlieren images. Images made by Erica Kaminski.
     12'''''Magnetic field lines oriented in the x-direction and their interaction with a hypersonic clumpy flow.''''' A Mach-25 speed wind is continuously injected into the grid from the left where it encounters and disperses a field of denser rings of gas clumps. The dynamic interplay between the clumps, shocks, and magnetic field is illustrated in these synthetic schlieren images.
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    18 '''''Magnetic field lines oriented in the y-direction and their interaction with a hypersonic clumpy flow.''''' A Mach-25 speed wind is continuously injected into the grid from the left where it encounters and disperses a field of denser rings of gas clumps. The dynamic interplay between the clumps, shocks, and magnetic field is illustrated in these synthetic schlieren images. In contrast to the Bx case, it is found that magnetic field lines oriented in y act to inhibit the dispersal of the clumps. The result is a thick wall of compacted gas and shocks that sweeps up the field as it traverses the grid. Images made by Erica Kaminski.
     18'''''Magnetic field lines oriented in the y-direction and their interaction with a hypersonic clumpy flow.''''' A Mach-25 speed wind is continuously injected into the grid from the left where it encounters and disperses a field of denser rings of gas clumps. The dynamic interplay between the clumps, shocks, and magnetic field is illustrated in these synthetic schlieren images. In contrast to the Bx case, it is found that magnetic field lines oriented in y act to inhibit the dispersal of the clumps. The result is a thick wall of compacted gas and shocks that sweeps up the field as it traverses the grid.
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    22 [[Image(ByDense_Schlieren.png)]]
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    24 [[BR]]
    25 '''A binary stellar system in a common envelope evolution phase. The white central star blows a spherical wind, orange scale, which swallows the orbiting black star companion''.
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    2822[[Image(binary0002.jpeg)]]
     
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    5751[[Image(rotatingLEVELS.gif)]]
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     54* [EricasJournalPics Erica's Research Journal Images]