Mar 8, 2017
Visualization of the 3-D structure of plasma turbulence in a tokamak and in the ionosphere. Credit: Greg Foss, TACC.
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Visualization of the 3-D structure of plasma turbulence in a tokamak and in the ionosphere. Credit: Greg Foss, TACC.
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🌞🧪 La sonda Parker Solar Probe ha alcanzado cotas sin precedentes cerca del Sol, “besando” su atmósfera y permitiendo medir directamente cómo el viento solar se calienta y acelera a partir de plasma y campos magnéticos complejos. Estas observaciones están reescribiendo nuestro entendimiento de la transferencia energética en la heliosfera.
coronal mass ejection of June 7, 2011, over and over and over
Wonderful pictures of magnified Snowflakes...
Snowflakes can tell us a great deal about the structural organisation of water at an atomic level. Their fractal nature appears to fit the rules of plasma dynamics, which can be demonstrated at any scale.
Each and every snowflake is a completely unique little fractal, demonstrating imperfect, yet self-similar symmetry.
Even if you don't care about the Science, they look mighty fine...