BASED ON A
NASA/GSFC PRESS
RELEASE
Dec. 13, 1999: From May 10-12,
1999, the solar wind that blows constantly from the Sun virtually
disappeared -- the most drastic and longest-lasting decrease
ever observed.
Dropping to a fraction of its normal density and to half its
normal speed, the solar wind died down enough to allow physicists
to observe particles flowing directly from the Sun's corona to
Earth. This severe change in the solar wind also changed the
shape of Earth's magnetic field and produced an unusual auroral
display at the North Pole.
Right: Data visualization of the
X ray emissions over the North Pole during the "polar rain"
of electrons on May 11, 1999. The emissions were detected by
the PIXIE instrument on NASA's Polar spacecraft. [larger
image]
Starting late on May 10 and continuing through the early
hours of May 12, NASA's ACE and Wind spacecraft each observed
that the density of the solar wind dropped by more than 98%.
Because of the decrease, energetic electrons from the Sun were
able to flow to Earth in narrow beams, known as the strahl. Under
normal conditions, electrons from the Sun are diluted, mixed,
and redirected in interplanetary space and by Earth's magnetic
field (the magnetosphere). But in May 1999, several satellites
detected electrons arriving at Earth with properties similar
to those of electrons in the Sun's corona, suggesting that they
were a direct sample of particles from the Sun.
"This event provides a window to see the Sun's corona directly,"
said Dr. Keith Ogilvie, project scientist for NASA's Wind spacecraft
and a space physicist at NASA's Goddard Space Flight Center,
Greenbelt, MD. "The beams from the corona do not get broken
up or scattered as they do under normal circumstances, and the
temperature of the electrons is very similar to their original
state on the Sun."
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"Normally, our view of the corona from Earth is like
seeing the Sun on an overcast, cloudy day," said Dr. Jack
Scudder, space physicist from the University of Iowa and principal
investigator for the Hot Plasma Analyzer on NASA's Polar spacecraft.
"On May 11, the clouds broke and we could see clearly."
Left: This pair of images in visible light
from the Polar satellite's Visible Imaging System compares the
northern auroral regions on May 11, 1999, and a more typical
day on November 13, 1999. Credit: University of Iowa/NASA. [larger image]
Fourteen years ago, Scudder and Dr. Don Fairfield of Goddard
predicted the details of an event such as occurred on May 11,
saying that it would produce an intense "polar rain"
of electrons over one of the polar caps of Earth. The polar caps
typically do not receive enough energetic electrons to produce
visible aurora. But in an intense polar rain event, Scudder and
Fairfield theorized, the "strahl" electrons would flow
unimpeded along the Sun's magnetic field lines to Earth and precipitate
directly into the polar caps, inside the normal auroral oval.
Such a polar rain event was observed for the first time in May
when Polar detected a steady glow over the North Pole in X-ray
images.
In parallel with the polar rain event, Earth's magnetosphere
swelled to five to six times its normal size. NASA's Wind, IMP-8,
and Lunar Prospector spacecraft, the Russian INTERBALL satellite
and the Japanese Geotail satellite observed the most distant
bow shock ever recorded by satellites. Earth's bow shock is the
shock front where the solar wind slams into the sunward edge
of the magnetosphere.
Right: Animation -The Day the Solar Wind Disappeared
(Berry animation 9.4MB) As the solar wind dissipates on May 11,
1999, the magnetosphere and bow shock around Earth expand to
five times their normal size. The aurora, which usually forms
ovals around Earth's poles, fills in over the northern polar
cap. Credit: NASA [Quicktime
movie]
According to observations from the ACE spacecraft, the density
of helium in the solar wind dropped to less than 0.1% of its
normal value, and heavier ions, held back by the Sun's gravity,
apparently could not escape from the Sun at all. Data from NASA's
SAMPEX spacecraft reveal that in the wake of this event, Earth's
outer electron radiation belts dissipated and were severely depleted
for several months afterward.
"The May event provides unique conditions to test ideas
about solar-terrestrial interactions," Ogilvie noted. "It
also strengthens our belief that we're beginning to understand
how the Sun-Earth connection works."
A NASA Video File relating to this story will air on December
13 at Noon EDT. NASA Television is available on GE-2, transponder
9C at 85 degrees West longitude, with vertical polarization.
Frequency is on 3880.0 megahertz, with audio on 6.8 megahertz.
Video File Advisories can be found at ftp://ftp.hq.nasa.gov/pub/pao/tv-advisory/nasa-tv.txt
Left: This movie, which can span
from 2 to 6 hours of actual time, shows the most recent images
of the Earth's auroral region taken from space by the Ultraviolet
Imager (UVI) Instrument on board the POLAR spacecraft. New movies
are generated every 6 hours. Hit reload for the latest animation
or visit the UVI
aurora home page for new pictures every 7 minutes. |