Christian Harris (@iamchrisharris)
PUT YOUR BEARD IN MY MOUTH
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if i look back, i am lost
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Origami Around
Color Me Curious
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❣ Chile in a Photography ❣
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NASA
Cookie Run:Kingdom Official!

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Jar Jar Binks Fan Club
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@thinkingmanproject
Christian Harris (@iamchrisharris)
California Waves - Santa Cruz, USA - Sammy Garcia(@sammy_garcia)
Geometry
Know the neighbors- All 9 planets (Yes 9, we love Pluto- Deal with it)(NASA Images)
Tokyo, Japan - Lukasz Palka(@lkazphoto)
Sunsets/Sunrises in S.E. Queensland, Auatralia - Ben Mulder (@benmuldersunsets)
Jessie Graff (@jessiegraffpwr)
Kyoto, Japan - Tetsu (@tetsu6o6)
4-stroke engine - Matt Mikka
Amandine Henry (@amandine_henry)
Brooke Wells (@brookewellss)
Tembea- Kenya
Photo by Shaun Mousley (@Shaunmousley)
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Automotive Photography - Zach Brehl (@Zachbrehl) Vintage Mercedes Benz, Barn Find.
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Automotive Photography - Zach Brehl (@Zachbrehl) Vintage Mercedes Benz, Barn Find.
More at thinkingmanproject.com
How exactly the solar wind plasma is heated is a hot topic in space physics, because it is hotter than expected for an expanding gas and almost no collisions are present. Scientists have suggested that the cause of this heating may be hidden in the turbulent character of the solar wind plasma.
Advanced supercomputer simulations are helping to understand these complex motions: the image shown here is from one such simulation. It represents the distribution of the current density in the turbulent solar wind plasma, where localised filaments and vortices have appeared as a consequence of the turbulent energy cascade. The blue and yellow colours show the most intense currents (blue for negative and yellow for positive values). (Source ESA.int)
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