Ricardocedillob - Sin Título

More Posts from Ricardocedillob and Others

3 years ago

Sabías que... en 1958 en la Bahía de Lituya (Alaska) se produjo el Tsunami más grande jamás datado?

Y es que llegó a medir la friolera de 524 metros de altura, llegando a ser llamado el megatsunami más grande de la historia.

Para hacerte a la idea, casi cubriría la última planta del Burj Khalifa (584 mts del total de 830mts que mide)

2 years ago

Puppies in the snow

8 years ago
I Got Pressured Into Playing Undertale (sweats A Little) I Don’t Wanna Have A Bad Time….

I got pressured into playing Undertale (sweats a little) I don’t wanna have a bad time….

7 years ago
A Visual Explanation Of The Process Of Evolution.
A Visual Explanation Of The Process Of Evolution.
A Visual Explanation Of The Process Of Evolution.
A Visual Explanation Of The Process Of Evolution.

A visual explanation of the process of Evolution.

7 years ago
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature

The upper atmosphere of the Sun is dominated by plasma filled magnetic loops (coronal loops) whose temperature and pressure vary over a wide range. The appearance of coronal loops follows the emergence of magnetic flux, which is generated by dynamo processes inside the Sun. Emerging flux regions (EFRs) appear when magnetic flux bundles emerge from the solar interior through the photosphere and into the upper atmosphere (chromosphere and the corona). The characteristic feature of EFR is the Ω-shaped loops (created by the magnetic buoyancy/Parker instability), they appear as developing bipolar sunspots in magnetograms, and as arch filament systems in Hα. EFRs interact with pre-existing magnetic fields in the corona and produce small flares (plasma heating) and collimated plasma jets. The GIFs above show multiple energetic jets in three different wavelengths. The light has been colorized in red, green and blue, corresponding to three coronal temperature regimes ranging from ~0.8Mk to 2MK. 

Image Credit: SDO/U. Aberystwyth

8 years ago
Catherine Deneuve 

Catherine Deneuve 

2 months ago
ricardocedillob - Sin título
ricardocedillob - Sin título
ricardocedillob - Sin título

Inter 175A Berline 1955. - source Moto Vitelloni - Wheels n' wings.

3 years ago
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ricardocedillob - Sin título
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