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REPORT SSDTR8992Observations of LargeAmplitude, WhistlerModeWave Ducts in the Outer PlasmasphereH. C. KOONSSpace Sciences Laboratory Operations The Aerospace Corporation El Segundo, CA 9024500 0)(12February
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01
Determine the frequency range of the whistler-mode observations.
02
Record the start and end times of each observation.
03
Note the location (latitude and longitude) of where the observations were made.
04
Measure the peak amplitude of the whistler-mode signals.
05
Document any additional information such as background noise levels or interference.

Who needs observations of large-amplitude whistler-mode?

01
Researchers studying magnetospheric dynamics and wave-particle interactions.
02
Scientists investigating plasma physics and space weather phenomena.
03
Engineers developing technologies for communications and satellite systems.
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Observations of large-amplitude whistler-mode are reports detailing the presence and characteristics of whistler-mode waves with high amplitudes.
Researchers and scientists studying electromagnetic waves in the Earth's magnetosphere are required to file observations of large-amplitude whistler-mode.
Observations of large-amplitude whistler-mode can be filled out by documenting the wave characteristics, time of occurrence, location, and any relevant measurements.
The purpose of observations of large-amplitude whistler-mode is to better understand the behavior and effects of whistler-mode waves in the Earth's magnetosphere.
Information such as wave frequency, amplitude, polarization, propagation direction, occurrence time, and location must be reported on observations of large-amplitude whistler-mode.
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