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  • richardmitnick 12:57 pm on October 14, 2017 Permalink | Reply
    Tags: “Nanoflares” may be responsible for the corona’s extreme temperatures, Hard X-rays, , , Nanoflares, , NASA Sounding Rocket Instrument Spots Signatures of Long-Sought Small Solar Flares, NASA UC Berkeley FOXSI sounding rocket, One of the consequences of nanoflares would be pockets of superheated plasma, ,   

    From Goddard: “NASA Sounding Rocket Instrument Spots Signatures of Long-Sought Small Solar Flares” 

    NASA Goddard Banner
    NASA Goddard Space Flight Center

    Oct. 13, 2017
    Sarah Frazier
    sara.frazier@nasa.gov
    NASA’s Goddard Space Flight Center, Greenbelt, Md.

    Like most solar sounding rockets, the second flight of the FOXSI instrument – short for Focusing Optics X-ray Solar Imager – lasted 15 minutes, with just six minutes of data collection. But in that short time, the cutting-edge instrument found the best evidence to date of a phenomenon scientists have been seeking for years: signatures of tiny solar flares that could help explain the mysterious extreme heating of the Sun’s outer atmosphere.

    FOXSI detected a type of light called hard X-rays – whose wavelengths are much shorter than the light humans can see – which is a signature of extremely hot solar material, around 18 million degrees Fahrenheit. These kinds of temperatures are generally produced in solar flares, powerful bursts of energy. But in this case, there was no observable solar flare, meaning the hot material was most likely produced by a series of solar flares so small that they were undetectable from Earth: nanoflares. The results were published Oct. 9, 2017, in Nature Astronomy.

    “The key to this result is the sensitivity in hard X-ray measurements,” said Shin-nosuke Ishikawa, a solar physicist at the Japan Aerospace Exploration Agency, or JAXA, and lead author on the study. “Past hard X-ray instruments could not detect quiet active regions, and combination of new technologies enables us to investigate quiet active regions by hard X-rays for the first time.”

    1
    The NASA-funded FOXSI instrument captured new evidence of small solar flares, called nanoflares, during its December 2014 flight on a suborbital sounding rocket. Nanoflares could help explain why the Sun’s atmosphere, the corona, is so much hotter than the surface. Here, FOXSI’s observations of hard X-rays are shown in blue, superimposed over a soft X-ray image of the Sun from JAXA and NASA’s Hinode solar-observing satellite.
    Credits: JAXA/NASA/

    JAXA/NASA HINODE spacecraft


    NASA UC Berkeley JAXA FOXSI sounding rocket

    These observations are a step toward understanding the coronal heating problem, which is how scientists refer to the extraordinarily – and unexpectedly – high temperatures in the Sun’s outer atmosphere, the corona. The corona is hundreds to thousands of times hotter than the Sun’s visible surface, the photosphere. Because the Sun produces heat at its core, this runs counter to what one would initially expect: normally the layer closest to a source of heat, the Sun’s surface, in this case, would have a higher temperature than the more distant atmosphere.

    “If you’ve got a stove and you take your hand farther away, you don’t expect to feel hotter than when you were close,” said Lindsay Glesener, project manager for FOXSI-2 at the University of Minnesota and an author on the study.

    The cause of these counterintuitively high temperatures is an outstanding question in solar physics. One possible solution to the coronal heating problem is the constant eruption of tiny solar flares in the solar atmosphere, so small that they can’t be directly detected. In aggregate, these nanoflares could produce enough heat to raise the temperature of the corona to the millions of degrees that we observe.

    One of the consequences of nanoflares would be pockets of superheated plasma. Plasma at these temperatures emits light in hard X-rays, which are notoriously difficult to detect. For instance, NASA’s RHESSI satellite – short for Reuven Ramaty High Energy Solar Spectroscopic Imager – launched in 2002, uses an indirect technique to measure hard X-rays, limiting how precisely we can pinpoint the location of superheated plasma. But with the cutting-edge optics available now, FOXSI was able to use a technique called direct focusing that can keep track of where the hard X-rays originate on the Sun.

    “It’s really a completely transformative way of making this type of measurement,” said Glesener. “Even just on a sounding rocket experiment looking at the Sun for about six minutes, we had much better sensitivity than a spacecraft with indirect imaging.”

    FOXSI’s measurements – along with additional X-ray data from the JAXA and NASA Hinode solar observatory – allow the team to say with certainty that the hard X-rays came from a specific region on the Sun that did not have any detectable larger solar flares, leaving nanoflares as the only likely instigator.

    “This is a proof of existence for these kinds of events,” said Steve Christe, the project scientist for FOXSI at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and an author on the study. “There’s basically no other way for these X-rays to be produced, except by plasma at around 10 million degrees Celsius [18 million degrees Fahrenheit]. This points to these small energy releases happening all the time, and if they exist, they should be contributing to coronal heating.”

    There are still questions to be answered, like: How much heat do nanoflares actually release into the corona?

    “This particular observation doesn’t tell us exactly how much it contributes to coronal heating,” said Christe. “To fully solve the coronal heating problem, they would need to be happening everywhere, even outside of the region observed here.”

    Hoping to build up a more complete picture of nanoflares and their contribution to coronal heating, Glesener is leading a team to launch a third iteration of the FOXSI instrument on a sounding rocket in summer 2018. This version of FOXSI will use new hardware to eliminate much of the background noise that the instrument sees, allowing for even more precise measurements.

    A team led by Christe was also selected to undertake a concept study developing the FOXSI instrument for a possible spaceflight as part of the NASA Small Explorers program.

    FOXSI is a collaboration between the United States and JAXA. The second iteration of the FOXSI sounding rocket launched from the White Sands Missile Range in New Mexico on Dec. 11, 2014. FOXSI is supported through NASA’s Sounding Rocket Program at the Goddard Space Flight Center’s Wallops Flight Facility in Virginia. NASA’s Heliophysics Division manages the sounding rocket program.

    Related:

    JAXA press release on these findings (Japanese)
    NASA-funded FOXSI to Observe X-rays from Sun
    https://www.nasa.gov/mission_pages/sounding-rockets/index.html

    See the full article here.

    Please help promote STEM in your local schools.

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    Stem Education Coalition

    NASA’s Goddard Space Flight Center is home to the nation’s largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe.

    Named for American rocketry pioneer Dr. Robert H. Goddard, the center was established in 1959 as NASA’s first space flight complex. Goddard and its several facilities are critical in carrying out NASA’s missions of space exploration and scientific discovery.


    NASA/Goddard Campus

     
  • richardmitnick 12:38 pm on October 9, 2017 Permalink | Reply
    Tags: , , “Nanoflares” may be responsible for the corona’s extreme temperatures, , , Explosions on the sun’s surface explain its extremely hot outermost layers, ,   

    From Science: “Explosions on the sun’s surface explain its extremely hot outermost layers” 

    AAAS
    Science

    Oct. 9, 2017
    Katherine Kornei

    1
    NASA/JPL-Caltech/GSFC

    This summer’s total solar eclipse revealed rare views of the sun’s corona, its outermost layers of plasma millions of degrees in temperature. But the solar corona has long baffled scientists: Why is it so searingly hot compared with the sun’s visible surface, which is about 1000 times cooler? Now, researchers have suggested that relatively small explosions known as “nanoflares” may be responsible for the corona’s extreme temperatures. Working in the New Mexico desert, the scientists launched a sounding rocket called FOXSI containing seven telescopes on a 15-minute trip into space to observe the sun (shown above in x-ray light).

    2
    NASA FOXSI soounding rocket

    The telescopes, with more sensitive detectors than previous x-ray telescopes, recorded high-energy light indicative of temperatures exceeding 10 million°C from one region of the sun. But solar flares—the brief, intense flashes of light caused by the sun’s magnetic fields changing shape suddenly—couldn’t be causing the heating because none were observed. Instead, many nanoflares, a million times weaker than traditional solar flares but still packing enough of a punch to meet the United States’ energy needs for a year, were acting in concert to heat the corona, the team reports today in Nature Astronomy. Upcoming FOXSI launches and other space-based telescopes may reveal more about nanoflares, the researchers suggest.

    See the full article here .

    Please help promote STEM in your local schools.

    STEM Icon

    Stem Education Coalition

     
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