Ricardocedillob - Sin Título

ricardocedillob - Sin título

More Posts from Ricardocedillob and Others

4 years ago

OMFG

Ha pasado de pinchar en las rave de valencia a tocar directos con la guitarra

7 years ago
Did You Know?

Did you know?

7 years ago
The Helium Atom

The Helium Atom

Helium nuclei were created in the Big Bang and contain two protons and two neutrons each. Helium is the second most abundant element, comprising roughly one quarter of the mass of the Universe. This animation zooms into a standard helium atom, showing its protons (green), neutrons (white), and electrons (blue).

Credits: Dana Berry / Lead Animator Michael McClare (HTSI)

7 years ago
By Jaccob McKay

by Jaccob McKay

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4 months ago
4 years ago

Ludwig van Beethoven - Moonlight Sonata ( 3rd Movement ) Tina S Cover 

Beethoven “Moonlight” Sonata,  III “Presto Agitato” Valentina Lisitsa

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

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ricardocedillob - Sin título
Sin título

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