Hurricanes Have No Place To Hide, Thanks To Better Satellite Forecasts

Hurricanes Have No Place to Hide, Thanks to Better Satellite Forecasts

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If you’ve ever looked at a hurricane forecast, you’re probably familiar with “cones of uncertainty,” the funnel-shaped maps showing a hurricane’s predicted path. Thirty years ago, a hurricane forecast five days before it made landfall might have a cone of uncertainty covering most of the East Coast. The result? A great deal of uncertainty about who should evacuate, where it was safe to go, and where to station emergency responders and their equipment.

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Over the years, hurricane forecasters have succeeded in shrinking the cone of uncertainty for hurricane tracks, with the help of data from satellites. Polar-orbiting satellites, which fly nearly directly above the North and South Poles, are especially important in helping cut down on forecast error.

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The orbiting electronic eyeballs key to these improvements: the Joint Polar Satellite System (JPSS) fleet. A collaborative effort between NOAA and NASA, the satellites circle Earth, taking crucial measurements that inform the global, regional and specialized forecast models that have been so critical to hurricane track forecasts.

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The forecast successes keep rolling in. From Hurricanes Harvey, Irma and Maria in 2017 through Hurricanes Florence and Michael in 2018, improved forecasts helped manage coastlines, which translated into countless lives and property saved. In September 2018, with the help of this data, forecasters knew a week ahead of time where and when Hurricane Florence would hit. Early warnings were precise enough that emergency planners could order evacuations in time — with minimal road clogging.  The evacuations that did not have to take place, where residents remained safe from the hurricane’s fury, were equally valuable.

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The satellite benefits come even after the storms make landfall. Using satellite data, scientists and forecasters monitor flooding and even power outages. Satellite imagery helped track power outages in Puerto Rico after Hurricane Maria and in the Key West area after Hurricane Irma, which gave relief workers information about where the power grid was restored – and which regions still lacked electricity. 

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Flood maps showed the huge extent of flooding from Hurricane Harvey and were used for weeks after the storm to monitor changes and speed up recovery decisions and the deployment of aid and relief teams.

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As the 2019 Atlantic hurricane season kicks off, the JPSS satellites, NOAA-20 and Suomi-NPP, are ready to track hurricanes and tropical cyclones as they form, intensify and travel across the ocean – our eyes in the sky for severe storms. 

For more about JPSS, follow @JPSSProgram on Twitter and facebook.com/JPSS.Program, or @NOAASatellites on Twitter and facebook.com/NOAASatellites.

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

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5 years ago

Lol

rulandtafego - Ruland Yuandris Tafego
rulandtafego - Ruland Yuandris Tafego
5 years ago

Bangga lihat adik-adik pemuda yg punya semangat dan antusias menyambut Natal tahun ini. Berdoa utk generasi muda saat ini supaya menjadi generasi yg mencintai Tuhan. Amen! 😊😇👍👍👍


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5 years ago

I AM BLESSING 😇😇🙏🙏💪💪

"Jika kamu berkata negatif, kamu tidak bisa berharap hidup yg positif. Jika perkataanmu buruk, hidupmu juga akan buruk." (Ps. Joel Osteen)

3 years ago
 Aku Sangat Menyukai Pantai.
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5 years ago

Three Ways to Travel at (Nearly) the Speed of Light

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One hundred years ago, Einstein’s theory of general relativity was supported by the results of a solar eclipse experiment. Even before that, Einstein had developed the theory of special relativity — a way of understanding how light travels through space.

Particles of light — photons — travel through a vacuum at a constant pace of more than 670 million miles per hour.

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All across space, from black holes to our near-Earth environment, particles are being accelerated to incredible speeds — some even reaching 99.9% the speed of light! By studying these super fast particles, we can learn more about our galactic neighborhood. 

Here are three ways particles can accelerate:

1) Electromagnetic Fields!

Electromagnetic fields are the same forces that keep magnets on your fridge! The two components — electric and magnetic fields — work together to whisk particles at super fast speeds throughout the universe. In the right conditions, electromagnetic fields can accelerate particles at near-light-speed.

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We can harness electric fields to accelerate particles to similar speeds on Earth! Particle accelerators, like the Large Hadron Collider and Fermilab, use pulsed electromagnetic fields to smash together particles and produce collisions with immense amounts of energy. These experiments help scientists understand the Big Bang and how it shaped the universe!

2) Magnetic Explosions!

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Magnetic fields are everywhere in space, encircling Earth and spanning the solar system. When these magnetic fields run into each other, they can become tangled. When the tension between the crossed lines becomes too great, the lines explosively snap and realign in a process known as magnetic reconnection. Scientists suspect this is one way that particles — for example, the solar wind, which is the constant stream of charged particles from the Sun — are sped up to super fast speeds.

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When magnetic reconnection occurs on the side of Earth facing away from the Sun, the particles can be hurled into Earth’s upper atmosphere where they spark the auroras.

3) Wave-Particle Interactions!

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Particles can be accelerated by interactions with electromagnetic waves, called wave-particle interactions. When electromagnetic waves collide, their fields can become compressed. Charged particles bounce back and forth between the waves, like a ball bouncing between two merging walls. These types of interactions are constantly occurring in near-Earth space and are responsible for damaging electronics on spacecraft and satellites in space.

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Wave-particle interactions might also be responsible for accelerating some cosmic rays from outside our solar system. After a supernova explosion, a hot, dense shell of compressed gas called a blast wave is ejected away from the stellar core. Wave-particle interactions in these bubbles can launch high-energy cosmic rays at 99.6% the speed of light.

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

5 years ago
vc
she is beautiful 😍
Gamlaha beach
Gamlaha beach 2

I thank my God, every time I remember you. (Phil. 1:3 ) 😇❤

Step by step we are moving forward


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5 years ago

John dan Carol McGuirk - Perancis - Gereja Paris Dan Acara Amal Untuk Tuna Wisma Di Tengah Tragedi Pemboman Prancis

John dan Carol McGuirk – Perancis – Gereja Paris Dan Acara Amal Untuk Tuna Wisma Di Tengah Tragedi Pemboman Prancis

Sabtu pagi, 14 November 2015, kami bangun di kota yang sangat sunyi. Biasanya, kota sudah bising dengan suara orang-orang berangkat ke kantor, mengerjakan pekerjaan rumah, membawa anak-anak ke sekolah, membawa anjing jalan-jalan, bertemu teman-teman, atau ikut kegiatan seni yang selalu ada di sekitar kami di kota yang indah ini. Namun, kemarin, suasana sangat sepi. Sepi yang aneh. Orang-orang…

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5 years ago

Wowo😃👍👍😍

Dolphins are so smart

5 years ago

Jangan mengisi hati dan hidup anda dengan air comberan! 👍🏼👍🏼

3 years ago

Seeing your smile is happiness for me. Meanwhile, having you is the most beautiful gift in my life.

I thank my God every time I remember you. (Filipi 1:3)


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