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Sunday, March 13, 2016

Performer, Anonymous Bosh Theatre Co.

Description. Anonymous Bosh Theatre are looking for two actors for script development and performances of their new production Let's Get Ready To ...

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Standardize Summary, Help text fields for anonymous and authenticated roles.

As of now there are no summary text for anonymous and authenticated roles, So its better to add summary text fields for anonymous and authenticated ...

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Ocean City, MD's surf is at least 5.42ft high

Maryland-Delaware, March 14, 2016 at 09:00AM

Ocean City, MD Summary
At 3:00 AM, surf min of 4.02ft. At 9:00 AM, surf min of 5.42ft. At 3:00 PM, surf min of 5.22ft. At 9:00 PM, surf min of 4.42ft.

Surf maximum: 5.64ft (1.72m)
Surf minimum: 5.42ft (1.65m)
Tide height: 0.78ft (0.24m)
Wind direction: SSW
Wind speed: 8.4 KTS


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The Flash Spectrum of the Sun


In a flash, the visible spectrum of the Sun changed from absorption to emission on March 9 during the total solar eclipse. That fleeting moment, at the beginning the total eclipse phase, is captured by telephoto lens and diffraction grating in this image from clearing skies over Ternate, Indonesia. At left, the overwhelming light from the Sun is just blocked by the lunar disk. The normally dominant absorption spectrum of the solar photosphere is hidden. What remains, spread by the diffraction grating into the spectrum of colors to the right of the eclipsed Sun, are individual eclipse images. The images appear at each wavelength of light emitted by atoms along the thin visible arc of the solar chromosphere and in an enormous prominence extending beyond the Sun's upper limb. The brightest images, or strongest chromospheric emission lines, are due to Hydrogen atoms that produce the red hydrogen alpha emission at the far right and blue hydrogen beta emission to the left. In between, the bright yellow emission image is caused by atoms of Helium, an element only first discovered in the flash spectrum of the Sun. via NASA http://ift.tt/1pma33F

Inside Cyclone Winston (February 20, 2016)

The NASA GPM satellite passed directly over Tropical Cyclone Winston just after it made landfall on the north coast of Viti Levu Island, which is the largest and most populated island in the nation of Fiji. At the time, Winston was one of the most intense tropical cyclones observed in the South Pacific Ocean, and took an unusual track on the way to Fiji, completing a large counter-clockwise loop during the preceding week. NASA's GPM satellite is designed to measure rainfall using both passive microwave (GMI) and radar (DPR) instruments. GMI measuremensts are sensitive to the column-integrated rain and ice water, and cover a wide swath, whereas the DPR can observe 3D structures of radar signals reflected by rain and snow in a narrower swath. In this animation, the GMI rainfall estimates are shown at the Earth's surface below the 3D storm structure revealed by DPR.

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