Search Publications

Measurement of the Electric Fluctuation Spectrum of Magnetohydrodynamic Turbulence
DOI: 10.1103/PhysRevLett.94.215002 Bibcode: 2005PhRvL..94u5002B

Bale, S. D.; Horbury, T. S.; Reme, H. +2 more

Magnetohydrodynamic (MHD) turbulence in the solar wind is observed to show the spectral behavior of classical Kolmogorov fluid turbulence over an inertial subrange and departures from this at short wavelengths, where energy should be dissipated. Here we present the first measurements of the electric field fluctuation spectrum over the inertial and…

2005 Physical Review Letters
Cluster 476
Gamma-Ray Constraint on Galactic Positron Production by MeV Dark Matter
DOI: 10.1103/PhysRevLett.94.171301 Bibcode: 2005PhRvL..94q1301B

Bertone, Gianfranco; Beacom, John F.; Bell, Nicole F.

The Galactic positrons, as observed by their annihilation gamma-ray line at 0.511 MeV, are difficult to account for with astrophysical sources. It has been proposed that they are produced instead by dark matter annihilation or decay in the inner Galactic halo. To avoid other constraints, these processes are required to occur “invisibly,” such that…

2005 Physical Review Letters
INTEGRAL 210
Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements
DOI: 10.1103/PhysRevLett.95.231101 Bibcode: 2005PhRvL..95w1101M

Dasso, S.; Matthaeus, W. H.; Smith, C. W. +3 more

Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary …

2005 Physical Review Letters
Cluster 198
Weak Compressible Magnetohydrodynamic Turbulence in the Solar Corona
DOI: 10.1103/PhysRevLett.95.265004 Bibcode: 2005PhRvL..95z5004C

Chandran, Benjamin D. G.

This Letter presents a calculation of the power spectra of weakly turbulent Alfvén waves and fast magnetosonic waves (“fast waves”) in low-β plasmas. It is shown that three-wave interactions transfer energy to high-frequency fast waves and, to a lesser extent, high-frequency Alfvén waves. High-frequency waves produced by MHD turbulence are a promi…

2005 Physical Review Letters
SOHO 126
Drift-Kinetic Alfvén Waves Observed near a Reconnection X Line in the Earth's Magnetopause
DOI: 10.1103/PhysRevLett.95.065002 Bibcode: 2005PhRvL..95f5002C

Balogh, A.; Reme, H.; Goldstein, M. L. +7 more

We identify drift-kinetic Alfvén waves in the vicinity of a reconnection X line on the Earth’s magnetopause. The dispersive properties of these waves have been determined using wavelet interferometric techniques applied to multipoint observations from the Cluster spacecraft. Comparison of the observed wave dispersion with that expected for drift-k…

2005 Physical Review Letters
Cluster 93
Ion-Pressure Equations Derived from Measurements in Space
DOI: 10.1103/PhysRevLett.95.015004 Bibcode: 2005PhRvL..95a5004S

Stasiewicz, K.

Cluster measurements at the bow shock, the magnetosheath, and the magnetospheric boundary layer are used to derive ion-pressure equations for hot anisotropic plasmas. It is demonstrated that both perpendicular and parallel ion pressures are well approximated by polybaric expressions ∝NγBκ, where N is the plasma density, B is …

2005 Physical Review Letters
Cluster 18
Proper Orthogonal Decomposition of Solar Photospheric Motions
DOI: 10.1103/PhysRevLett.95.061102 Bibcode: 2005PhRvL..95f1102V

Vecchio, A.; Carbone, V.; Veltri, P. +5 more

The spatiotemporal dynamics of the solar photosphere is studied by performing a proper orthogonal decomposition (POD) of line of sight velocity fields computed from high resolution data coming from the MDI/SOHO instrument. Using this technique, we are able to identify and characterize the different dynamical regimes acting in the system. Low-frequ…

2005 Physical Review Letters
SOHO 16