Search Publications

Large-scale electron acceleration by parallel electric fields during magnetic reconnection
DOI: 10.1038/nphys2249 Bibcode: 2012NatPh...8..321E

Egedal, J.; Daughton, W.; Le, A.

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.

2012 Nature Physics
Cluster 194
Observations and simulations of non-local acceleration of electrons in magnetotail magnetic reconnection events
DOI: 10.1038/nphys1903 Bibcode: 2011NatPh...7..360A

Hwang, Kyoung-Joo; Kivelson, Margaret G.; Schriver, David +6 more

Magnetic reconnection in magnetized plasmas represents a change in magnetic field topology and is associated with a concomitant energization of charged particles that results from a conversion of magnetic energy into particle energy. In Earth's magnetosphere this process is associated with the entry of the solar wind into the magnetosphere and wit…

2011 Nature Physics
Cluster 155
The effect of flares on total solar irradiance
DOI: 10.1038/nphys1741 Bibcode: 2010NatPh...6..690K

Schmutz, Werner; de Wit, Thierry Dudok; Mekaoui, Sabri +3 more

Flares are powerful bursts of energy released by relatively poorly understood processes that take place in the atmospheres of stars. However, although solar flares, from our own Sun, are the most energetic events in the solar system, in comparison to the total output of the Sun they are barely noticeable. Consequently, the total amount of radiant …

2010 Nature Physics
SOHO 37
Planetary physics: Under the spell of the rings
DOI: 10.1038/nphys1849 Bibcode: 2010NatPh...6..841T

Trabesinger, Andreas

2010 Nature Physics
Cassini 0
Observation of energetic electrons within magnetic islands
DOI: 10.1038/nphys777 Bibcode: 2008NatPh...4...19C

Daly, P. W.; Khotyaintsev, Y.; Vaivads, A. +10 more

Magnetic reconnection is the underlying process that releases impulsively an enormous amount of magnetic energy in solar flares , flares on strongly magnetized neutron stars and substorms in the Earth's magnetosphere. Studies of energy release during solar flares, in particular, indicate that up to 50% of the released energy is carried by accelera…

2008 Nature Physics
Cluster 229
In situ evidence of magnetic reconnection in turbulent plasma
DOI: 10.1038/nphys574 Bibcode: 2007NatPh...3..236R

André, M.; Vaivads, A.; Owen, C. J. +3 more

Magnetic reconnection is a universal process leading to energy conversion in plasmas. It occurs in the Solar System, in laboratory plasmas and is important in astrophysics . Reconnection has been observed so far only at large-scale boundaries between different plasma environments . It is not known whether reconnection occurs and is important in tu…

2007 Nature Physics
Cluster 298
Satellite observations of separator-line geometry of three-dimensional magnetic reconnection
DOI: 10.1038/nphys650 Bibcode: 2007NatPh...3..609X

Escoubet, C. P.; Dandouras, I.; Glassmeier, K. -H. +14 more

Detection of a separator line that connects magnetic nulls and the determination of the dynamics and plasma environment of such a structure can improve our understanding of the three-dimensional (3D) magnetic reconnection process. However, this type of field and particle configuration has not been directly observed in space plasmas. Here we report…

2007 Nature Physics
Cluster 53
In situ evidence for the structure of the magnetic null in a 3D reconnection event in the Earth's magnetotail
DOI: 10.1038/nphys342 Bibcode: 2006NatPh...2..478X

Escoubet, C. P.; Balogh, A.; Glassmeier, K. H. +12 more

Magnetic reconnection is one of the most important processes in astrophysical, space and laboratory plasmas. Identifying the structure around the point at which the magnetic field lines break and subsequently reform, known as the magnetic null point, is crucial to improving our understanding of reconnection. But owing to the inherently three-dimen…

2006 Nature Physics
Cluster 108
Cosmic-ray diffusion near the Bohm limit in the Cassiopeia A supernova remnant
DOI: 10.1038/nphys391 Bibcode: 2006NatPh...2..614S

Stage, M. D.; Allen, G. E.; Houck, J. C. +1 more

The acceleration of cosmic rays in our Galaxy by means of diffusive shock (Fermi) acceleration is believed to occur primarily in supernova remnants (SNRs). Despite considerable theoretical work, the precise details are still unknown, in part because of the difficulty in directly observing nucleons that are accelerated to TeV energies in-and affect…

2006 Nature Physics
Suzaku 53
Astrophysics: Fingerprints in Saturn's F ring
DOI: 10.1038/nphys161 Bibcode: 2005NatPh...1...87H

Hamilton, Douglas P.

A planet's rings can be distorted by the gravitational pull of its satellites, and these complex interactions have been difficult to disentangle. Saturn's moon Prometheus, however, has now been caught returning to the scene of the crime.

2005 Nature Physics
Cassini 1