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Caption: NASA’s Solar Dynamics Observatory (SDO) captured this image of an M5.7 class flare on May 3, 2013 at 1:30 p.m. EDT. This image shows light in the 131 Angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal.
Caption: NASA’s Solar Dynamics Observatory (SDO) captured this image of an M5.7 class flare on May 3, 2013 at 1:30 p.m. EDT. This image shows light in the 131 Angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal.
Credit: NASA/Goddard/SDO
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The sun emitted a mid-level solar flare, peaking at 1:32 pm EDT on May 3, 2013. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel. This disrupts the radio signals for as long as the flare is ongoing, and the radio blackout for this flare has already subsided.
This flare is classified as an M5.7 class flare. M-class flares are the weakest flares that can still cause some space weather effects near Earth. Increased numbers of flares are quite common at the moment, since the sun's normal 11-year activity cycle is ramping up toward solar maximum, which is expected in late 2013.
Updates will be provided as they are available on the flare and whether there was an associated coronal mass ejection (CME), another solar phenomenon that can send solar particles into space and affect electronic systems in satellites and on Earth.
NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.
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Captured just with the light emitted from the mobile phone, do share your comments, critiques and opinion on this capture...
Caption: NASA’s Solar Dynamics Observatory (SDO) captured this image of an M5.7 class flare on May 3, 2013 at 1:30 p.m. EDT. This image shows light in the 131 Angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal.
Caption: NASA’s Solar Dynamics Observatory (SDO) captured this image of an M5.7 class flare on May 3, 2013 at 1:30 p.m. EDT. This image shows light in the 131 Angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal.
Credit: NASA/Goddard/SDO
---
The sun emitted a mid-level solar flare, peaking at 1:32 pm EDT on May 3, 2013. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel. This disrupts the radio signals for as long as the flare is ongoing, and the radio blackout for this flare has already subsided.
This flare is classified as an M5.7 class flare. M-class flares are the weakest flares that can still cause some space weather effects near Earth. Increased numbers of flares are quite common at the moment, since the sun's normal 11-year activity cycle is ramping up toward solar maximum, which is expected in late 2013.
Updates will be provided as they are available on the flare and whether there was an associated coronal mass ejection (CME), another solar phenomenon that can send solar particles into space and affect electronic systems in satellites and on Earth.
NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.
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iss067e191368 (July 24, 2022) --- At right, the Canadarm2 robotic arm maneuvers the Earth Surface Mineral Dust Source Investigation, or EMIT, after retrieving it from the trunk of the SpaceX Dragon cargo craft. EMIT was installed on ExPRESS Logistics Carrier-1 (top center) on the port side of the International Space Station's truss structure. The station's main solar arrays are also seen extending from the port truss segment. EMIT is a mineral dust source observation experiment that explores the Earth’s mineral dust cycle.
Mount Bromo (Indonesian: Gunung Bromo), is an active volcano caldera and part of the Tengger massif, in East Java, Indonesia. The Volcano has several eruptive centres from which it emits clouds of sulphurous steam.
--- in Dutch ---
Bromo (Indonesisch : Gunung Bromo), is een actieve vulkaan caldera en maakt deel uit van het Tengger massief in Oost Java, Indonesië. De vulkaan spuugt voortdurende stoom wolken uit die zwavel bevatten.
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EXPLORE Dec. 12 ~ #103
[ Bill Fontana - American, born 1947 ]
Sonic Shadows
2010 - Sound sculpture :12 channel live sound installation with 12 accelerometers, 8 loudspeakers, and 4 ultrasonic emitters on pan-tilt heads.
5305 emits a lot of the black stuff as it climbs past Oakworth Mound with the 14:45 ex-Keighley. 3rd May 1993.
Unrest at Turrialba Volcano, Costa Rica
Turrialba Volcano, located in central Costa Rica, emits a translucent plume of volcanic gases in this natural-color satellite image from January 21, 2010. According to the RED Sismológica Nacional (Costa Rican National Seismological Network), activity at the volcano increased markedly on January 4, 2010. Strong, long-lasting volcanic tremors were accompanied by gas plumes over the volcano, and emissions of ash began on January 5th. The “jet-type noise” of gas and ash rushing out of fumaroles was heard several kilometers away. On January 21, Nacion.com reported that potato and carrot farmers were asked to leave fields near the volcano’s summit due to further increases in gas emissions.
The barren summit region of the 3,340-meter- (10,960-foot-) high Turrialba appears gray and brown, while the volcanic plume is a hazy blue. Fields and pastures are light green, in contrast to dark green forest that covers the high-elevation ridges. Since 2007, frequent acid rain showers caused by activity at the volcano killed or damaged much of the vegetation to the southwest of the summit, leaving the area brown and orange. This image was acquired by the Advanced Land Imager (ALI) aboard NASA’s Earth Observing-1 (EO-1) satellite.
Credit: NASA Earth Observatory
Read more, high res: earthobservatory.nasa.gov/NaturalHazards/view.php?id=42425
NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.
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The magnetic field of our Milky Way Galaxy as seen by ESA’s Planck satellite. This image was compiled from the first all-sky observations of polarised light emitted by interstellar dust in the Milky Way. The magnetic field is displayed using a visualisation technique called line integral convolution (LIC).
Darker regions correspond to stronger polarised emission, and the striations indicate the direction of the magnetic field projected on the plane of the sky. The dark band running horizontally across the centre corresponds to the Galactic Plane. Here, the polarisation reveals a regular pattern on large angular scales, which is due to the magnetic field lines being predominantly parallel to the plane of the Milky Way. The data also reveal variations of the polarisation direction within nearby clouds of gas and dust. This can be seen in the tangled features above and below the plane, where the local magnetic field is particularly disorganised.
The image is a Mollweide projection of the full celestial sphere, with the plane of the Galaxy aligned with the horizontal axis of the oval. Certain areas in the image, mostly at high Galactic latitude, have been masked out. The overall intensity in these regions is low, complicating the separation of foreground and CMB components. Further data analysis will improve this by the time of the full data release in late 2014.
Full story: www.esa.int/Our_Activities/Space_Science/Planck/Planck_ta...
Credit: ESA and the Planck Collaboration
Virga clouds emit a "dry rain" which never makes it to the ground. Tucson -- Arizona
Please do not use this image on websites, blogs or other media without my explicit permission. © All rights reserved
My entry for the MSFC on Eurobricks it's a micro dio of a Beam emitter complete with a tiny Pelican dropship from Halo.
© Todos los derechos reservados. De compartir esta foto deberá ser con enlace directo a esta página.
Pues como ya es un clásico la unión del CTBA con la luna aquí está la de noviembre. Y esta foto tambien la han emitido en el tiempo de TVE en la 1. Aparece junto a Júpiter, en la izquierda, que está estos días en conjunción con ella. Otra luna llena en Madrid.
Emit w/ Mike Graves
Terminal Kings is 10 days and 10 nights of Street Art, music, performance and energy presented by the University of Denver in a proud partnership with Denver International Airport.
Artists included Sam Flores, David Choe and Highraff.
Emitting a great plume of smoke as it passes... destimnation blind reads Longbrisge, but it's not clear if this is a passenger service or an ECS move.
This is an odd formation of what appears to be 116 DMBS, 116 DMS, 116 DMS, 115 DMBS (smaller brake compartment) and 116 DMS, though it's possible the second and last vehicles could be Class 117 or 118. With no trailer vehicles, this would have been a powerful formation of 1,660hp, assuming all ten engines were operational (the Class 115 engines were 230hp each).
Probably early 1990s, at a time when the cross-city electrification was behind schedule, so formations of DMU power cars were assembled in an attempt to keep to EMU schedules.
Scanned from a 35mm colour negative. Was slide 8406.
09/11/2013 1309
In a way! :-)
I just arrived back home from my trip to El Paso and wanted to get this out there tonight to hopefully meet the deadline for the LightPaintingPhotography.com website contest.
Now that I am home, I will be able to get back on getting costs together for the Digital Light Wand and return all the inquiry emails on that. And maybe fit a little more LP in this weekend! :-)
Light Painting - Single Exposure.
The Giant Sky Wheel is a giant travelling Ferris wheel currently located in Birrarung Marr Reserve in Melbourne.
The Ferris wheel is illuminated by more than 300,000 light emitting diodes, which provide an amazing light show at night.
(http://www.photologium.com/melbourne_night/ferris_wheel_birrarung_marr_03.html)
Emitting a huge plume of smoke across the valley, visiting Thompson B1 no. 61264 blasts away from Irwell Vale Halt with the 10.00 Heywood to Rawtenstall service on the 11th January 2014. The previous night's frost is still evident on the ground on this very chilly and windy morning.
Cameron and I met up with another Flickr photographer this evening (blonboy) to give him some insight on our LP techniques. I was mainly going to go out and test a few new orb tools that I created to see how they would work out. Had a great time out!
Light Painting - Single Exposure