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I could read this love story all day










Chiara Bautista’s beautiful art! She is amazing and probably my favorite artist :)
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Heather Penn - http://happydorid.tumblr.com - https://twitter.com/heatpenn - https://www.kickstarter.com/projects/607081461/tea-spirits-2015-calendar - https://www.inprnt.com/gallery/happydorid - https://dribbble.com/fastbee - https://www.instagram.com/heatpenn
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Casimir Lee - http://casimir0304.cgsociety.org - https://www.facebook.com/CaSiMiR0304 - http://casimir0304.deviantart.com
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Sheena Liam aka シーナ・リアム aka Sheena Liam Yue Sheen aka 粘悦馨 aka Nián Yuèxīn (Malaysian-Chinese, b. 1991, Subang Jaya, Selangor, Malaysia) - Top Fashion Model and Embroiderer. Embroidery Arts: Black Thread, Embroidery Hoop
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“Learn to see light”. That’s what cinematographer Julio Macat told me when I asked him how to get better at photography. He explained that beautiful light doesn’t only exist at sunrise and sunset, it’s around us constantly but we aren’t looking for it. This shot was taken in a small strip between a messy kitchen and messy living room. The light from the patio was coming in and illuminating a sliver not much wider than Julie. It was so much brighter than the room that when I exposed for it, everything else fell to black. pentax 67 | tri-x | Indie Film Lab
www.ryanmuirhead.com
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The Van Allen Belt & the South Atlantic Anomaly
NASA’s first satellite, launched in 1958, discovered two giant swaths of radiation encircling Earth. Five decades later, scientists are still trying to unlock the mysteries of these phenomena known as the Van Allen belt. The belt is named after its discoverer, American astrophysicist James Van Allen.
The near-Earth space environment is a complex interaction between the planet’s magnetic field, cool plasma moving up from Earth’s ionosphere, and hotter plasma coming in from the solar wind. This dynamic region is populated by charged particles (electrons and ions) which occupy regions known as the plasmasphere and the Van Allen radiation belt. As solar wind and cosmic rays carry fast-moving, highly energized particles past Earth, some of these particles become trapped by the planet’s magnetic field. These particles carry a lot of energy, and it is important to mention their energies when describing the belt, because there are actually two distinct belts; one with energetic electrons forming the outer belt, and a combination of protons and electrons creating the inner belt. The resulting belts, can swell or shrink in size in response to incoming particles from Earth’s upper atmosphere and changes in the solar wind. Recent studies suggest that there is boundary at the inner edge of the outer belt at roughly 7,200 miles in altitude that appears to block the ultrafast electrons from breaching the invisible shield that protects Earth.
Earth’s magnetic field doesn’t exactly line up with the planet’s rotation axis, the belts are actually tilted a bit. Because of this asymmetry, one of the shields that trap potentially harmful particles from space dips down to 200 km (124 mi) altitude.
This dip in the earth’s magnetic field allows charged particles and cosmic rays to reach lower into the atmosphere. Satellites and other low orbiting spacecraft passing through this region of space actually enter the Van Allen radiation belt and are bombarded by protons. Exposure to such radiation can wreak havoc on satellite electronics, and pose serious health risks to astronauts. This peculiar region is called the South Atlantic Anomaly.
Credit: NASA/ESA/M. Kornmesser
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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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Once upon a time in the West, Hayley Eichenbaum
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