Geomagnetosphere
activity |
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2.7
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Chorus
recorded by Cluster 2 satellite from data collected on July 9,
2001. Chorus consists of brief, rising-frequency tones that
sound like the chorus of birds singing at sunrise, hence the
name "chorus" or "dawn chorus". Chorus at
Earth is generated by electrons in Earth's Van Allen radiation
belts. Once generated, the chorus waves affect the motions of
the electrons through a process called a wave-particle
interaction. Wave-particle interactions disturb the
trajectories of the radiation belt electrons and cause the
electrons to hit the upper atmosphere. Document Donald
A. Gurnett/U/Iowa. |
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1.5
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"Saucers"
recorded by Dynamics Explorer spacecraft. Document Donald
A. Gurnett/U/Iowa. |
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803
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Short
but spectacular whistler recorded by Cluster 3 and 4
satellites from data collected on Feb 4, 2001. Whistlers are
produced by lightning. This energy is radiated as
electromagnetic waves over a very broad spectrum of
frequencies, from very low-frequency radio waves to visible
light. Some of these radio waves propagate upward into the
ionized gas located above the Earth's atmosphere guided along
geomagnetic field, and often echo back and forth between the
northern and southern hemispheres. The waves travel faster at
higher frequencies and slower at lower frequencies. Therefore,
a spacecraft will first detect the higher frequencies and
later the lower frequencies. The result is a whistling tone,
hence the name "whistler". Document Donald
A. Gurnett/U/Iowa.
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807
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Pure
whistlers of lightnings recorded with a VLF receiver. The note
whistler has traveled along a signal magnetic field line. It
is heard as a clear whistling sound. Pulses that we heard over
10 kHz at beginning, at 8 and 9 sec are OMEGA signals. Several
other faint whislters are audible in the sound sample. These
whistlers are sferics dispersed even more than tweeks. The
sound of a whistler is a musical descending tone that lasts
for a second or more. The high frequencies arrive first,
followed by lower ones. Document IMAGE/INSPIRE.
Additional
information can be found on Stephen
P. McGreevy's website. |
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246
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Lightning
whistlers propagating in the magnetosphere. Lightning-generated whistlers came into
regular use as remote probes of the radial distribution of
electron density in the Earth's geomagnetic equatorial plane. |
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899
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Diffuse
whistlers. The signals traveled along a set of magnetic field
lines that are not all of the same length. The sound is
"breathy" or "swooshy". Document IMAGE/INSPIRE. |
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240
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Sferics,
short for "atmospherics", are impulsive signals
emitted by lightnings striking within a thousand kilometers or
so of the receiver. Their signals cover simultaneous all audio
VLF frequencies. Document IMAGE/INSPIRE. |
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891
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Whistle
echo trains. They result when the radio wave bounces back and
forth between magnetic conjugate points. Each time the signal
bounces off the ionosphere, some of the energy leaks down in
the lower atmosphere and is heard as a whistler. All of the
whistlers in the train are the result of a single lightning
stroke. Successive "hops" of the whistler are seen
with increasing dispersion time as the distance travelled
grows with each bounce. Document IMAGE/INSPIRE. |
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1.3
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Two-hop
whistlers originated near the receiver site. The signal that
travels along the magnetic field line bounces off the
ionosphere in the other magnetic hemisphere and returns to be
heard as a whistler near where the original lightning stroke
occurred. Two-hop whistlers can be identified by the presence
of a strong "local" sferic (within 2000 km) between
one and two seconds before the whistler is heard. Document IMAGE/INSPIRE. |
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Spectacular
whistlings recorded in NW Alberta, Canada, on June 2, 1996 at
approx. 1030 UTC (4.30 a.m. MDT). Pitched whistling and whooping
are wildly varying upward and downward. |
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474
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Pure
whistlers recorded during a beautiful colorful dawn at Great
Basin National Park on Sept 16, 1994. Taped using a WR-4B VLF
receiver connected to a 150-meter longwire (500 ft.) strung to
the north-east at about 2-4m (6-15 ft) above the ground in the
aspen and fir trees. These whistlers and associated lightning
sferics were probably occurring from nasty T-storms pummeling
Dallas, Texas and eastern Nebraska (Omaha area). The
geomagnetic indices were also rather low (A=6-7, K=0-1, SFI~80). Additional information can be found on Stephen
P. McGreevy's website. Document McGreevy. |
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T-storms.
They are multitude of very hissy (diffuse) whistlers recorded
on June 13, 1993 near Berlin, Nevada at approx. 1330 UTC
(local dawn) with a
WR-4B VLP receiver conencted to 5 meters (15 ft) vertical
wire. Additional information can be found on Stephen
P. McGreevy's website. Document McGreevy. |
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329
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Nice
mix of pure whistlers and tweeks that occurred all night.
Recorded on April 1, 1994 at 11:30 UTC (3h30 a.m. PST), 160 km
north of San Francisco, CA, in Mendocino County. Additional
information can be found on Stephen
P. McGreevy's website. Document McGreevy. |
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313
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Magnetosphere
whistlers recorded on the nightside on March 26, 1996 at 07:59
UTC by Don Gurnett
from U.Iowa.
Initially the wideband receiver (VLF) was connected to the
electric Eu antenna, but was switched to the Bu magnetic
search coil antenna at 07:59:06 UTC. A series of brief
whistlers is evident throughout this interval below 1.5 kHz.
These sounds are audio frequency electromagnetic waves
produced by lightning. Once produced, these waves travel along
closed magnetic field lines from one hemisphere to the other
in the right-hand polarized, whistler mode of propagation. The
duration of the whistling tone is related to the length of the
propagation path. Because of anisotropies in the index of
refraction, the wave energy is confined within a cone that
makes an angle of 19°28' with respect to the local magnetic
field. |
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249
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Magnetosphere
whistlers recorded on May 10, 1996 at 00:16 UTC by Don
Gurnett from U.Iowa
using a wideband spectrogram taken from the Earth dayside. The
wideband receiver was connected to a magnetic loop antenna
throughout this interval. Two clusters of whistlers of varying
duration are seen below 8 kHz at 00:16:25 UTC and 00:16:44 UTC. |
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609
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Magnetosphere
whistlers recorded on June 12, 1996 at 13:58 UTC by Don
Gurnett from U.Iowa
using a wideband spectrogram taken from the Earth nightside.
The wideband receiver was again connected to a magnetic loop
antenna. Some whistlers can be seen up to 9 kHz (13:58:24 UTC and
13:58:29 UTC) and several more below 4 kHz (13:58:32 UTC and
13:58:44 UTC). |
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240
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Lightning
whistlers and tweeks propagating in the magnetosphere
recorded by NASA
scientists. |
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294
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Lightning
whistlers propagating in the magnetosphere recorded by NASA
scientists. |
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450
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Whistlers
in the magnetosphere.
Document U.Iowa. |
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269
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Lightning
whistlers recorded in stereo.
Document U.Iowa. |
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Earth
proton whistlers.
Document U.Iowa. |
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665
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Earth
multi-hop whistlers.
Document U.Iowa. |
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216
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Lightning
tweeks recorded between 100 Hz and 30 kHz by Altaïr. |
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873
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Magnetosphere
cusp waves recorded on May 29, 1996 at 02:56 UTC by Don
Gurnett from U.Iowa.
The magnetic field lines of the Earth can be divided into two
parts according to their location on the sunward or tailward
side of the planet. Between these two parts on both
hemispheres are funnel-shaped areas with near zero magnetic
field magnetitude called the polar cusps. They provide a
direct entry for the magnetosheath plasma into the
magnetosphere. |
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609
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Magnetosphere
chorus recorded on May 31, 1996 at 06:47 UTC by
Don Gurnett
from U.Iowa.
Chorus emissions are
electromagnetic widebands emissions propagating in the
right-hand polarized whistler mode. They are among the most
intense plasma waves in the outer magnetosphere. Chorus
emissions are observed at intermediate invariant latitudes,
between L=4 and L=10, and over a wide range of local times
with a peak in the distribution near local dawn. This
record was taken at daytime at latitudes just below the
dayside auroral zone. The receiver was connected to a magnetic
loop antenna. The discrete tones characteristic of chorus can
be seen as a dense population of short, very intense rising
tones between 500 Hz and 1.2 kHz. |
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881
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Chorus.
Occasionally, especially in the quiet times of the morning,
chorus can be heard. They sounds like many birds calling in
turn. Chorus seems to be the result of many brief, short-path
whistler-like emissions occurring at almost the same time.
Document IMAGE/INSPIRE. |
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367
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Loud
dawn chorus and hiss recorded on August 18, 1993 in SE
Oregon's Alvord Desert at 14:30 UTC (7h30 a.m. PDT). A major
magnetic storm was in progress. Magnetic field
"micro-pulsations" are very evident (slow
undulations in the hiss/chorus every 3-4 sec similar to ocean
waves. Additional information can be found on Stephen
P. McGreevy's website. Document McGreevy. |
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345
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Dawn
chorus with evident magnetic field micro-pulsations
(undulations in the chorus trains). Recorded by Michael Mideke
in 1990 or 1991. |
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663
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Geomagnetic
storm recorded on Feb 21, 1994 by Southpole. |
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396
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Earth
chorus.
Document U.Iowa. |