• A new look at sunspots

    From ScienceDaily@1337:3/111 to All on Fri Oct 9 21:30:46 2020
    A new look at sunspots

    Date:
    October 9, 2020
    Source:
    NASA/Goddard Space Flight Center
    Summary:
    NASA's extensive fleet of spacecraft allows scientists to study
    the Sun extremely close-up - one of the agency's spacecraft is
    even on its way to fly through the Sun's outer atmosphere. But
    sometimes taking a step back can provide new insight.



    FULL STORY ========================================================================== NASA's extensive fleet of spacecraft allows scientists to study the Sun extremely close-up -- one of the agency's spacecraft is even on its way
    to fly through the Sun's outer atmosphere. But sometimes taking a step
    back can provide new insight.


    ==========================================================================
    In a new study, scientists looked at sunspots -- darkened patches on the
    Sun caused by its magnetic field -- at low resolution as if they were
    trillions of miles away. What resulted was a simulated view of distant
    stars, which can help us understand stellar activity and the conditions
    for life on planets orbiting other stars.

    "We wanted to know what a sunspot region would look like if we couldn't
    resolve it in an image," said Shin Toriumi, lead author on the new study
    and scientist at ?the Institute of Space and Astronautical Science at
    JAXA. "So, we used the solar data as if it came from a distant star to
    have a better connection between solar physics and stellar physics."
    Sunspots are often precursors to solar flares -- intense outbursts of
    energy from the surface of the Sun -- so monitoring sunspots is important
    to understanding why and how flares occur. Additionally, understanding the frequency of flares on other stars is one of the keys to understanding
    their chance of harboring life. Having a few flares may help build up
    complex molecules like RNA and DNA from simpler building blocks. But
    too many strong flares can strip entire atmospheres, rendering a planet uninhabitable.

    To see what a sunspot and its effect on the solar atmosphere would look
    like on a distant star, the scientists started with high-resolution
    data of the Sun from NASA's Solar Dynamics Observatory and JAXA/NASA's
    Hinode mission. By adding up all the light in each image, the scientists converted the high- resolution images into single datapoints. Stringing subsequent datapoints together, the scientists created plots of how the
    light changed as the sunspot passed across the Sun's rotating face. These plots, which scientists call light curves, showed what a passing sunspot
    on the Sun would look like if it were many light-years away.

    https://www.youtube.com/watch?v=QJc1G8Zuqo8 "The Sun is our closest
    star. Using solar observing satellites, we can resolve signatures on
    the surface 100 miles wide," said Vladimir Airapetian, co-author on
    the new study and astrophysicist at NASA's Goddard Space Flight Center
    in Greenbelt, Maryland. "On other stars you might only get one pixel
    showing the entire surface, so we wanted to create a template to decode activity on other stars."


    ==========================================================================
    The new study, published in the Astrophysical Journal, looked at simple
    cases where there is just one group of sunspots visible across the entire
    face of the Sun. Even though NASA and JAXA missions have continually
    gathered observations of the Sun for over a decade, these cases are
    quite rare. Usually there are either several sunspots -- such as during
    the solar maximum, which we are now moving toward -- or none at all. In
    all the years of data, the scientists only found a handful of instances
    of just one isolated sunspot group.

    Studying these events, the scientists found the light curves differed when
    they measured different wavelengths. In visible light, when a singular
    sunspot appears at the center of the Sun, the Sun is dimmer. However,
    when the sunspot group is near the edge of the Sun, it's actually brighter
    due to faculae - - bright magnetic features around sunspots -- because,
    near the edge, the hot walls of their nearly vertical magnetic fields
    become increasingly visible.

    The scientists also looked at the light curves in x-ray and ultraviolet
    light, which show the atmosphere above the sunspots. As the atmospheres
    above sunspots are magnetically heated, the scientists found brightening
    there at some wavelengths. However, the scientists also unexpectedly
    discovered that the heating could also cause a dimming in the light coming
    from the lower temperature atmosphere. These findings may provide a tool
    to diagnose the environments of spots on the stars.

    "So far we've done the best-case scenarios, where there's only one sunspot visible," Toriumi said. "Next we are planning on doing some numerical
    modeling to understand what happens if we have multiple sunspots."
    By studying stellar activity on young stars in particular, scientists
    can glean a view of what our young Sun may have been like. This will
    help scientists understand how the young Sun -- which was overall more
    dim but active - - impacted Venus, Earth and Mars in their early days. It
    could also help explain why life on Earth started four billion years ago,
    which some scientists speculate is linked to intense solar activity.

    Studying young stars can also contribute to scientists' understanding of
    what triggers superflares -- those that are 10 to 1000 times stronger than
    the biggest seen on the Sun in recent decades. Young stars are typically
    more active, with superflares happening almost daily. Whereas, on our
    more mature Sun, they may only occur once in a thousand years or so.

    Spotting young suns that that are conducive to supporting habitable
    planets, helps scientists who focus on astrobiology, the study of the
    origin evolution, and distribution of life in the universe. Several next generation telescopes in production, which will be able to observe other
    stars in x-ray and ultraviolet wavelengths, could use the new results
    to decode observations of distant stars.

    In turn, this will help identify those stars with appropriate levels
    of stellar activity for life -- and that can then be followed up by observations from other upcoming high-resolution missions, such as NASA's
    James Webb Space Telescope.


    ========================================================================== Story Source: Materials provided by
    NASA/Goddard_Space_Flight_Center. Original written by Mara
    Johnson-Groh. Note: Content may be edited for style and length.


    ==========================================================================


    Link to news story: https://www.sciencedaily.com/releases/2020/10/201009121852.htm

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