I Wanna Go. So Beautiful!!!!

I wanna go. So beautiful!!!!

Mt. Tam

More Posts from Amyleigh81 and Others

amyleigh81

7 years ago

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amyleigh81

4 years ago

Lips of All Colors

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amyleigh81

2 years ago

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amyleigh81

4 years ago

Love & Hope

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amyleigh81

7 years ago

High Heel Bowl...Love it!!

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amyleigh81

8 years ago

We Just Got An Unprecedented Look At A Black Hole Ripping Apart A Star

We just got an unprecedented look at a black hole ripping apart a star

For the first time ever, astronomers got a close-up peek at a black hole ripping apart a star, a rare event that results in some of the star’s material getting ejected out into space. To research this phenomenon, astronomers used data from a tidal disruption that happened 3.9 billion years ago. Studying tidal disruptions like this one is revealing new information about how black holes behave.

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amyleigh81

7 years ago

Chill the Fuck Out!

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amyleigh81

7 years ago

Cosmic Geometric Skull

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amyleigh81

7 years ago

Red Pot Leaf

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amyleigh81

7 years ago

Absolutely amazing!!

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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