One. More. Month: Our Guide to the Total Solar Eclipse (USA)

Binary_Bark

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Have you heard?

I remember, getting into astronomy as a kid back in the 1970s, building a pinhole projector in a shoe box and watching the partial solar eclipse of February 26th, 1979 from our living room in northern Maine. I had no Learjet, no magic carpet to whisk me off to that thin thread of a path of totality way out west along the Pacific coast. As I settled for the 66% partial solar eclipse, I remember news reports stating that a total solar eclipse won’t cross the United States again until… August 21st, 2017.

That date is almost upon us now, only one month from this coming Friday.

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his total solar eclipse is one for the ages, THE big ticket event for 2017. Umbraphiles (those who chase eclipses) have been planning for this one for decades, and it’s already hard to find a room along the path. Fear not, as you only need to be within striking distance the day of the eclipse to reach totality, though expect the roads to be congested that Monday morn.

The eclipse is indeed the first time totality touches the contiguous (“lower 48”) United States since 1979, and the first total solar eclipse to cross the United States since almost a century ago on June 8th 1918. A total solar eclipse did cross Hawaii on July 11th, 1991.

Partial phases for the eclipse begin at 15:47 Universal Time (UT) and span 5 hours and 18 minutes until 21:04 UT. The partial aspect of the eclipse touches all continents except Antarctica and Australia. The 115 kilometer wide shadow of Earth’s moon (known as the umbra) first makes landfall over the Oregon coast at 17:16 UT /10:16 Pacific Daylight Saving time (PDT) and races eastward at 3,900 kilometers per second. The shadow touches 14 states, just briefly nicking Montana and Iowa. Maximum totality of 2 minutes, 40 seconds occurs near Carbondale, Illinois.

Read More At: https://www.universetoday.com/136440/one-month-guide-total-solar-eclipse/
 

Binary_Bark

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NASA looks to solar eclipse to help understand Earth's energy system

It was midafternoon, but it was dark in an area in Boulder, Colorado on Aug. 3, 1998. A thick cloud appeared overhead and dimmed the land below for more than 30 minutes. Well-calibrated radiometers showed that there were very low levels of light reaching the ground, sufficiently low that researchers decided to simulate this interesting event with computer models. Now in 2017, inspired by the event in Boulder, NASA scientists will explore the moon's eclipse of the sun to learn more about Earth's energy system.
On Aug. 21, 2017, scientists are looking to this year's total solar eclipse passing across America to improve our modelling capabilities of Earth's energy. Guoyong Wen, a NASA scientist working for Morgan State University in Baltimore, is leading a team to gather data from the ground and satellites before, during and after the eclipse so they can simulate this year's eclipse using an advanced computer model, called a 3-D radiative transfer model. If successful, Wen and his team will help develop new calculations that improve our estimates of the amount of solar energy reaching the ground, and our understanding of one of the key players in regulating Earth's energy system, clouds.
Earth's energy system is in a constant dance to maintain a balance between incoming radiation from the sun and outgoing radiation from Earth to space, which scientists call the Earth's energy budget. The role of clouds, both thick and thin, is important in their effect on energy balance.
Like a giant cloud, the moon during the 2017 total solar eclipse will cast a large shadow across a swath of the United States. Wen and his team already know the dimensions and light-blocking properties of the moon, but will use ground and space instruments to learn how this large shadow affects the amount of sunlight reaching Earth's surface, especially around the edges of the shadow.


Read more at: https://phys.org/news/2017-07-nasa-solar-eclipse-earth-energy.html#jCp
 
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