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One
day in the fall of 2011, Neil Sheeley, a solar scientist at the Naval
Research Laboratory in Washington, D.C., did what he always does—look
through the daily images of the sun from NASA’s Solar Dynamics
Observatory (SDO).
But
on this day he saw something he’d never noticed before: a pattern of
cells with bright centers and dark boundaries occurring in the sun’s
atmosphere, the corona. These cells looked somewhat like a cell pattern
that occurs on the sun’s surface—similar to the bubbles that rise to the
top of boiling water—but it was a surprise to find this pattern higher
up in the corona, which is normally dominated by bright loops and dark
coronal holes.
Sheeley
discussed the images with his Naval Research Laboratory colleague Harry
Warren, and together they set out to learn more about the cells. Their
search included observations from a fleet of NASA spacecraft called the
Heliophysics System Observatory that provided separate viewpoints from
different places around the sun. They describe the properties of these
previously unreported solar features, dubbed “coronal cells,” in a paper
published online in The Astrophysical Journal on March 20, 2012 that will appear in print on April 10.
The
coronal cells occur in areas between coronal holes—colder and less
dense areas of the corona seen as dark regions in images—and “filament
channels” which mark the boundaries between sections of upward-pointing
magnetic fields and downward-pointing ones. Understanding how these
cells evolve can provide clues as to the changing magnetic fields at the
boundaries of coronal holes and how they affect the steady emission of
solar material known as the solar wind streaming from these holes.
“We
think the coronal cells look like flames shooting up, like candles on a
birthday cake,” says Sheeley. “When you see them from the side, they
look like flames. When you look at them straight down they look like
cells. And we had a great way of checking this out, because we could
look at them from the top and from the side at the same time using
observations from SDO, STEREO-A, and STEREO-B.”
When
the cells were discovered in the fall of 2011, the SDO and the two
STEREO (short for Solar Terrestrial Relations Observatory) spacecraft
each had widely different views of the sun. Thus, as the 27-day solar
rotation carried the coronal cells across the face of the sun, they
appeared first in STEREO-B data, then in SDO, and finally in STEREO-A,
before starting over again in STEREO-B. In addition, when one
observatory looked down directly on the cells, another observatory could
see them from the side.
The
researchers used time-lapse sequences obtained from the three
satellites to track these cells around the sun. When an observatory
looked down on one of these areas, it showed the cell pattern that
Sheeley first noticed. But when the same region was viewed obliquely, it
showed plumes leaning off to one side. Taken together, these
two-dimensional images reveal the three-dimensional nature of the cells
as columns of solar material extending upward through the sun’s
atmosphere, like giant pillars of gas.
To
round out the picture even further, the team turned to other
instruments and spacecraft. The original SDO images were from its
Atmospheric Imaging Assembly, which takes conventional images of the
sun. Another instrument on SDO, the Helioseismic and Magnetic Imager
(HMI), provides magnetic maps of the sun. The scientists superimposed
conventional images of the cells with HMI magnetic field images to
determine the placement of the coronal cells relative to the complex
magnetic fields of the sun’s surface.
First
of all, the magnetic field bundles lay centered inside the cells. This
represents a clear distinction between the coronal cells and another
well-known phenomenon known as supergranules. Supergranules also appear
as a large cell-like pattern on the sun’s surface, and their delineated
edges are created as the sideways motion of solar material sweeps weaker
magnetic fields toward their boundaries. Supergranules, therefore,
appear to have enhanced magnetic fields at their edges, while the
coronal cells show them at their centers.
Second,
the scientists learned more about how the coronal cells were related to
other structures on the sun, in their location between a coronal hole
and a nearby filament channel. The cells consistently occurred in areas
dominated by magnetic fields that point in a single direction, either up
or down. In addition, the fields of the nearby coronal hole are what’s
known as “open,” extending far into space without returning to the sun.
On the other hand, the field lines in the cells were “closed,” looping
up over the filament channel and connecting back down to the sun.
The
side-by-side nature of these open and closed magnetic fields—open in
the coronal holes, and closed in the coronal cells—led to another
scientific insight. In some of the movies, a large loop of solar
material called a “filament” erupted from the adjacent filament channel.
The coronal cells, with their closed field lines, disappeared and were
replaced with a dark coronal hole and its associated open field lines.
“Sometimes
the cells were gone forever, and sometimes they would reappear exactly
as they were,” says Sheeley. “So this means we need to figure out what’s
blowing out the candles on the birthday cake and re-lighting them. It’s
possible that this coronal cell structure is the same structure that
exists inside the coronal holes – but they’re visible to us when the
magnetic fields are closed, and not visible when the magnetic fields are
open.”
It
has long been known that isolated plumes occur intermittently inside
coronal holes when very small active regions erupt there. Presumably,
these eruptions are providing glimpses of discrete coronal structures
similar to the more permanently visible candles adjacent to the holes.
When a portion of a hole closes, the candle-like structure is suddenly
lit up by the appearance of cells.
In
addition to SDO and STEREO, the team went back to historical data on
ESA’s and NASA’s Solar and Heliospheric Observatory (SOHO), which has
provided observations since the previous sunspot minimum in 1996. They
did not find coronal cells in 1996 or in the years around the recent
sunspot minimum in 2008-2009, but they did find numerous examples of
cells in the years around the intervening sunspot maximum in 2000. The
recent increase in sunspot activity together with the improved
observations from STEREO and SDO may explain why the cells were
discovered in 2011.
The
team also constructed Doppler images—images that show how quickly and
where solar material in the sun’s atmosphere moves toward the viewer—of
the coronal cells using the Extreme-Ultraviolet Imaging Spectrometer
(EIS) on the Japanese Hinode spacecraft. These images show that the
centers of the cells move upward faster than their boundaries, further
rounding out the physical image of these giant candles with a section
rising from the middle.
“One
of the wonderful things about SDO is the way the observations can be
combined with other instruments,” says Dean Pesnell, SDO project
scientist at NASA’s Goddard Space Flight Center in Greenbelt, Md. ”
Combining data from SDO, STEREO, SOHO, and Hinode lets us paint a
picture of the whole sun in ways that one instrument can’t.”
The
discovery of coronal cells has already increased our knowledge of the
magnetic structure of the sun’s corona. In the future, studies of the
evolution of coronal cells may improve scientists’ understanding of the
magnetic changes at coronal-hole boundaries and their effects on the
solar wind and Earth’s space weather.
Source: NASA Goddard Space Flight Center
