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Article
| Open AccessTransmission of foreshock waves through Earth’s bow shock
The Earth’s bow shock results from the interaction of the solar wind with the terrestrial magnetic field. With global numerical simulations and spacecraft observations, the transmission of fast magnetosonic waves through the bow shock is revealed.
- L. Turc
- , O. W. Roberts
- & U. Ganse
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Article |
Structures in the terms of the Vlasov equation observed at Earth’s magnetopause
Insights into the structure of the Vlasov equation that governs the evolution of collisionless plasmas from observations have been limited. Now the spatial gradient term for electrons is analysed with recent data from the MMS mission.
- J. R. Shuster
- , D. J. Gershman
- & R. B. Torbert
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Letter |
Solar flare effects in the Earth’s magnetosphere
The solar wind affects the magnetosphere, but whether this holds true for solar flares was unclear. By combining geospace modelling with observations, solar flares are shown to influence the dynamics of the magnetosphere and its ionosphere coupling.
- Jing Liu
- , Wenbin Wang
- & Frederick Wilder
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Letter |
Near-Earth magnetotail reconnection powers space storms
Magnetic reconnection in the near-Earth magnetotail is observed to power a space storm, although suppression of magnetic reconnection caused by the Earth’s magnetic dipole was expected close to Earth.
- Vassilis Angelopoulos
- , Anton Artemyev
- & Yukinaga Miyashita
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Letter |
Plasmaspheric hiss waves generate a reversed energy spectrum of radiation belt electrons
Observations reveal that electrons in Earth’s outer radiation belt possess a spectrum that partially rises with increasing energy, contrary to common beliefs. Plasma hiss waves scattered off electrons are found to be the origin of this phenomenon.
- H. Zhao
- , B. Ni
- & A. J. Boyd
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Article |
Magnetotail energy dissipation during an auroral substorm
Substorms in the Earth’s magnetosphere lead to bright aurorae, releasing energy into the surrounding ionosphere. Ground- and space-based observations now reveal how that energy is dissipated and controlled by strong electric currents.
- E. V. Panov
- , W. Baumjohann
- & M. V. Kubyshkina
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Article |
Cross-scale energy transport in space plasmas
Processes in (space) plasmas occur on different levels — fluid, ion and electron. Now, from satellite data and simulations, an energy-transfer mechanism between the fluid and ion scales is reported: fluid velocity shear is converted into ion heating.
- T. W. Moore
- , K. Nykyri
- & A. P. Dimmock
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Article |
Explaining the dynamics of the ultra-relativistic third Van Allen radiation belt
The appearance of a third radiation belt in the Earth’s Van Allen belts is difficult to explain using existing models for two belts. However, a model based on ultra-low-frequency waves agrees quantitatively with measurements of the third belt.
- I. R. Mann
- , L. G. Ozeke
- & F. Honary
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Letter |
Coalescence of magnetic flux ropes in the ion diffusion region of magnetic reconnection
Merging magnetic flux ropes, which are believed to play an important role in magnetic reconnection, have now been clearly identified. Observations show that coalescence is indeed closely related to reconnection dynamics and also to turbulence.
- Rongsheng Wang
- , Quanming Lu
- & Shui Wang
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News & Views |
Reconnecting with two good friends
Two observational studies published in Nature Physics provided early evidence for the mechanisms of magnetic reconnection in three dimensions and in a turbulent medium.
- Ellen Zweibel
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Letter |
Cassini in situ observations of long-duration magnetic reconnection in Saturn’s magnetotail
Cassini’s encounter with Saturn’s magnetotail — the long magnetosphere region stretching into space — has revealed that plasma exits the magnetosphere through long-duration magnetic reconnection, which ejects ten times more mass than estimated.
- C. S. Arridge
- , J. P. Eastwood
- & M. K. Dougherty
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Article |
Secondary reconnection sites in reconnection-generated flux ropes and reconnection fronts
New three-dimensional simulations of magnetic reconnection suggest the existence of secondary reconnection sites that could be observed by the new NASA Magnetospheric MultiScale Mission.
- Giovanni Lapenta
- , Stefano Markidis
- & David L. Newman
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Letter |
Unusual stable trapping of the ultrarelativistic electrons in the Van Allen radiation belts
The Van Allen radiation belts are two rings of charged particles encircling the Earth. Therefore the transient appearance in 2012 of a third ring between the inner and outer belts was a surprise. A study of the ultrarelativistic electrons in this middle ring reveals new physics for particles above 2 MeV.
- Yuri Y. Shprits
- , Dmitriy Subbotin
- & Kyung-Chan Kim
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Letter |
Energetic electron acceleration by unsteady magnetic reconnection
Magnetic reconnection in the Earth's magnetosphere accelerates electrons. And yet energetic electrons are not created during reconnection in the solar wind. Observations from the Cluster spacecraft now suggest that electron acceleration is caused by repeated bursts of plasma flow, which only occur in situations where the magnetic reconnection is unsteady.
- H. S. Fu
- , Yu. V. Khotyaintsev
- & M. André
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News & Views |
Where did all the electrons go?
Geomagnetic storms driven by the solar wind can cause the flux of high-energy electrons in the Earth's Van Allen belts to rapidly fall. Analysis of data obtained during one such event from multiple spacecraft located at different altitudes in the magnetosphere reveals just where these electrons go.
- Mary K. Hudson
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Letter |
Large-scale electron acceleration by parallel electric fields during magnetic reconnection
Magnetic reconnection is a process by which the field lines of a magnetized plasma undergo dramatic realignment, releasing large amounts of energy. Large-scale simulations of reconnection events in the Earth’s magnetosphere suggest that this process takes place over much greater distances than previously expected.
- J. Egedal
- , W. Daughton
- & A. Le
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Letter |
Explaining sudden losses of outer radiation belt electrons during geomagnetic storms
Geomagnetic storms driven by the solar wind can cause a dramatic drop in the flux of high-energy electrons in the Earth’s outer Van Allen belt. Analysis of data obtained during such an event by three different sets of spacecraft suggests that these electrons are directed into space rather than lost to the atmosphere.
- Drew L. Turner
- , Yuri Shprits
- & Vassilis Angelopoulos