Plasmasphere

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The plasmasphere, or inner magnetosphere , is a region of the Earth's magnetosphere consisting of low-energy (cool) plasma. It is located above the ionosphere. The outer boundary of the plasmasphere is known as the plasmapause, which is defined by an order of magnitude drop in plasma density. In 1963 American scientist Don Carpenter and Soviet astronomer Konstantin Gringauz  [ ru ] proved the plasmasphere and plasmapause's existence from the analysis of very low frequency (VLF) whistler wave data. Traditionally, the plasmasphere has been regarded as a well behaved cold plasma with particle motion dominated entirely by the geomagnetic field and, hence, co-rotating with the Earth.

Contents

History

The discovery of the plasmasphere grew out of the scientific study of whistlers, natural phenomena caused by very low frequency (VLF) radio waves. Whistlers were first heard by radio operators in the 1890s. [1] British scientist Llewelyn Robert Owen Storey had shown lightning generated whistlers in his 1953 PhD dissertation. [1] [2] Around the same time, Storey had posited the existence of whistlers meant plasma was present in Earth's atmosphere, and that it moved radio waves in the same direction as Earth's magnetic field lines. [1] [2] From this he deduced but was unable to conclusively prove the existence of the plasmasphere. [2] In 1963 American scientist Don Carpenter and Soviet astronomer Konstantin Gringauz—independently of each other, and the latter using data from the Luna 2 spacecraft—experimentally proved the plasmasphere and plasmapause's existence, building on Storey's thinking. [1]

In 1965 Storey and French scientist M. P. Aubry worked on FR-1, a French scientific satellite equipped with instruments for measuring VLF frequencies and the local electron density of plasma. Aubry and Storey's studies of FR-1 VLF and electron density data further corroborated their theoretical models: VLF waves in the ionosphere occasionally passed through a thin layer of plasma into the magnetosphere, normal to the direction of Earth's magnetic field. [3] :1181 [4] Throughout the 1970s, Storey continued studying VLF waves using data gathered by FR-1. [2] Data received from the VLF receiver on OV3-3, launched 4 August 1966, determined the location of the plasmapause. [5]

In 2014 satellite observations from the THEMIS mission have shown that density irregularities such as plumes or biteouts may form. [6] [7] It has also been shown that the plasmasphere does not always co-rotate with the Earth. The plasma of the magnetosphere has many different levels of temperature and concentration. The coldest magnetospheric plasma is most often found in the plasmasphere. However, plasma from the plasmasphere can be detected throughout the magnetosphere because it gets blown around by the Earth's electric and magnetic fields. Data gathered by the twin Van Allen Probes show that the plasmasphere also limits highly-energetic ultrarelativistic electrons from cosmic and solar origin from reaching low earth orbits and the surface of the planet. [8] [9]

See also

Related Research Articles

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Llewelyn Robert Owen Storey is a British physicist and electrical engineer who has worked and lived most of his adult life in France. He is known for his research on the Earth's atmosphere, especially whistlers—very low frequency (VLF) radio waves caused by lightning strikes—and the plasmasphere. He was the first person to prove whistlers are caused by lightning strikes and to deduce the plasmasphere's existence. He was heavily involved in designing scientific instruments for FR-1, a 1965 French-American satellite, and subsequent studies and experiments using data FR-1 collected.

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<span class="mw-page-title-main">Dynamics Explorer 1</span> NASA satellite of the Explorer program

Dynamics Explorer 1 was a NASA high-altitude mission, launched on 3 August 1981, and terminated on 28 February 1991. It consisted of two satellites, DE-1 and DE-2, whose purpose was to investigate the interactions between plasmas in the magnetosphere and those in the ionosphere. The two satellites were launched together into polar coplanar orbits, which allowed them to simultaneously observe the upper and lower parts of the atmosphere.

<span class="mw-page-title-main">Dynamics Explorer 2</span> NASA satellite of the Explorer program

Dynamics Explorer 2 was a NASA low-altitude mission, launched on 3 August 1981. It consisted of two satellites, DE-1 and DE-2, whose purpose was to investigate the interactions between plasmas in the magnetosphere and those in the ionosphere. The two satellites were launched together into polar coplanar orbits, which allowed them to simultaneously observe the upper and lower parts of the atmosphere.

References

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  3. Aubry, M. P. (1968). "Some results of the FR-1 satellite experiment on the VLF wave field in the zone close to the transmitter". Journal of Atmospheric and Terrestrial Physics. 30 (6): 1161–1182. Bibcode:1968JATP...30.1161A. doi:10.1016/S0021-9169(68)80005-4.
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  8. "Star Trek-like invisible shield protects Earth from 'killer electrons' - Los Angeles Times". Los Angeles Times . 27 November 2014.
  9. "Plasma shield".

Further reading