Typhoon Power

Typhoon Power

The Typhoon Turbine Can Withstand Typhoon-force Winds And Convert The Energy Into Electricity. Its Inventor,

The typhoon turbine can withstand typhoon-force winds and convert the energy into electricity. Its inventor, Atsushi Shimizu, calculated that the captured energy from just one typhoon could power all of Japan for 50 years. Source

More Posts from F-taser-blog and Others

8 years ago

Why Do We Study Ice?

Discover why we study ice and how this research benefits Earth. 

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We fly our DC-8 aircraft very low over Antarctica as part of Operation IceBridge – a mission that’s conducting the largest-ever airborne survey of Earth’s polar ice.

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Records show that 2015 was the warmest year on record, and this heat affects the Arctic and Antarctica – areas that serve as a kind of air conditioner for Earth and hold an enormous of water.

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IceBridge flies over both Greenland and Antarctica to measure how the ice in these areas is changing, in part because of rising average global temperatures.

IceBridge’s data has shown that most of Antarctica’s ice loss is occurring in the western region. All that melting ice flows into the ocean, contributing to sea level rise.

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IceBridge has been flying the same routes since the mission began in 2009. Data from the flights help scientists better measure year-to-year changes.

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IceBridge carries the most sophisticated snow and ice instruments ever flown.  Its main instrument is called the Airborne Topographic Mapper, or ATM.The ATM laser measure changes in the height of the ice surface by measuring the time it takes for laser light to bounce off the ice and return to the plane – ultimately mapping ice in great detail, like in this image of Antarctica’s Crane Glacier.

Why Do We Study Ice?

For the sake of the laser, IceBridge planes have to fly very low over the surface of snow and ice, sometimes as low as 1,000 feet above the ground. For comparison, commercial flights usually stay around 30,000 feet! Two pilots and a flight enginner manage the many details involved in each 10- to 12-hour flight.

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One of the scientific radars that fly aboard IceBridge helped the British Antarctic Survey create this view of what Antarctica would look like without any ice.

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IceBridge also studies gravity using a very sensitive instrument that can measure minuscule gravitational changes, allowing scientists to map the ocean cavities underneath the ice edges of Antarctica. This data is essential for understanding how the ice and the ocean interact. The instrument’s detectors are very sensitive to cold, so we bundle it up to keep it warm!

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Though the ice sheet of Antarctica is two miles thick in places, the ice still “flows” – faster in some places and slower in others. IceBridge data helps us track how much glaciers change from year-to-year.

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Why do we call this mission IceBridge? It is bridging the gap between our Ice, Cloud and Land Elevation Satellite, or ICESat – which gathered data from 2003 to 2009 – and ICESat-2, which will launch in 2018.

Why Do We Study Ice?

Learn more about our IceBridge mission here: www.nasa.gov/icebridge and about all of our ice missions on Twitter at @NASA_Ice.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com


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8 years ago

Act good,now so that it would be beneficial in future


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8 years ago
Comet Outbursts
Comet Outbursts
Comet Outbursts
Comet Outbursts
Comet Outbursts

Comet outbursts

Although European Space Agency’s comet-landing mission Rosetta ended on 30 September, the data gathered through it will keep teaching us about comets for a while. 

Here are images taken by the Rosetta spacecraft’s camera when Comet 67P/Churyumov–Gerasimenko approached closest to the Sun in August. The comet became very active and outbursts occurred, a typical one thought to release 60–260 tonnes of material in just few minutes! 

The outburst can be divided into three categories based on how their dust flow looks like, and the outbursts occurred both when the Sun had started to warm up the previously shaded surface, and after illumination of a few hours. [1] So the outbursts could happen in at least two different ways.

Anyhow, they provide scientists insights of cometary lives and they look pretty cool. 

1. Summer fireworks on Rosetta’s comet.  23 September 2016

Copyright: OSIRIS: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM /DASP/IDA; NavCam: ESA/Rosetta/NavCam – CC BY-SA IGO 3.0


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8 years ago

Wifi evolve to LiFi 

post by worl of facts

Li-Fi Is The New Insanely Fast Wireless Internet

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Wi-Fi has revolutionized the experience of connecting online, but it has already been one-upped. The radiowave technology may be soon replaced with Li-Fi, the wireless internet alternative that is 100 times faster than the Wi-Fi we use today. 

Keep reading


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7 years ago
That's True

That's true

7 years ago

Oh I want something just like this....

Milky Way Over Vegas From Valley Of Fire [OC] [1365x2048] Visit Http://spaceviewsandbeyond.blogspot.com/2017/06/milky-way-over-vegas-from-valley-of.html

Milky Way Over Vegas from Valley of Fire [OC] [1365x2048] Visit http://spaceviewsandbeyond.blogspot.com/2017/06/milky-way-over-vegas-from-valley-of.html for more space pics


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8 years ago

HAPPY BDAY TO YOU:(post by DID-YOU-KNOW)

Every Year On August 5, The Mars Curiosity Rover Celebrates The Anniversary Of Its Arrival By Singing

Every year on August 5, the Mars Curiosity rover celebrates the anniversary of its arrival by singing the Happy Birthday song. To itself. All alone. On Mars. Source Source 2

Happy Birthday to the Curiosity rover! 

I had to post this in hopes that maybe it won’t be so lonely if we’re all thinking about… it.


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8 years ago

CHAKRAS (this is a post of cosmic portal,i like it very much)

Match This Understanding To Other Ancient Temples

Match this understanding to other ancient temples


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8 years ago

LETS DO IT TOGETHER NASA :)

Mission Possible: Redirecting an Asteroid

As part of our Asteroid Redirect Mission (ARM), we plan to send a robotic spacecraft to an asteroid tens of millions of miles away from Earth, capture a multi-ton boulder and bring it to an orbit near the moon for future crew exploration.

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This mission to visit a large near-Earth asteroid is part of our plan to advance the new technologies and spaceflight experience needed for a human mission to the Martian system in the 2030s.

How exactly will it work?

The robotic spacecraft, powered by the most advanced solar electric propulsion system, will travel for about 18 months to the target asteroid.

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After the spacecraft arrives and the multi-ton boulder is collected from the surface, the spacecraft will hover near the asteroid to create a gravitational attraction that will slightly change the asteroid’s trajectory.

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After the enhanced gravity tractor demonstration is compete, the robotic vehicle will deliver the boulder into a stable orbit near the moon. During the transit, the boulder will be further imaged and studied by the spacecraft.

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Astronauts aboard the Orion spacecraft will launch on the Space Launch System rocket to explore the returned boulder.

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Orion will dock with the robotic vehicle that still has the boulder in its grasp. 

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While docked, two crew members on spacewalks will explore the boulder and collect samples to bring back to Earth for further study.

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The astronauts and collected samples will return to Earth in the Orion spacecraft.

How will ARM help us send humans to Mars in the 2030s?

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This mission will demonstrate future Mars-level exploration missions closer to home and will fly a mission with technologies and real life operational constraints that we’ll encounter on the way to the Red Planet. A few of the capabilities it will help us test include: 

Solar Electric Propulsion – Using advanced Solar Electric Propulsion (SEP) technologies is an important part of future missions to send larger payloads into deep space and to the Mars system. Unlike chemical propulsion, which uses combustion and a nozzle to generate thrust, SEP uses electricity from solar arrays to create electromagnetic fields to accelerate and expel charged atoms (ions) to create a very low thrust with a very efficient use of propellant.

Trajectory and Navigation – When we move the massive asteroid boulder using low-thrust propulsion and leveraging the gravity fields of Earth and the moon, we’ll validate critical technologies for the future Mars missions. 

Advances in Spacesuits – Spacesuits designed to operate in deep space and for the Mars surface will require upgrades to the portable life support system (PLSS). We are working on advanced PLSS that will protect astronauts on Mars or in deep space by improving carbon dioxide removal, humidity control and oxygen regulation. We are also improving mobility by evaluating advances in gloves to improve thermal capacity and dexterity. 

Sample Collection and Containment Techniques – This experience will help us prepare to return samples from Mars through the development of new techniques for safe sample collection and containment. These techniques will ensure that humans do not contaminate the samples with microbes from Earth, while protecting our planet from any potential hazards in the samples that are returned. 

Rendezvous and Docking Capabilities – Future human missions to Mars will require new capabilities to rendezvous and dock spacecraft in deep space. We will advance the current system we’ve developed with the international partners aboard the International Space Station. 

Moving from spaceflight a couple hundred miles off Earth to the proving ground environment (40,000 miles beyond the moon) will allow us to start accumulating experience farther than humans have ever traveled in space.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com


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8 years ago
The Pleiades from Saaremaa, Estonia

The Pleiades from Saaremaa, Estonia

This image was taken by my friend Raivo Hein! Raivo has his own little observatory in Saaremaa, an Estonian island, and he has mastered astrophotography over the years. This brilliant view of the Pleiades or Seven Sisters was obtained with the exposure time of 8 hours by using the LRGB (Luminance, Red, Green and Blue) method.

As for technical details, ASA N12 Telescope, FLI MicroLine ML16200 Camera, and ASA DDM60 Pro Direct Drive Mount were used.

See more of his stunning images on Facebook & here on Tumblr.

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