Wave-vector dependence of magnetic-turbulence spectra in the solar wind

Physical Review Letters

Volumn 104, Issue 17, 2010, Pages

  Narita, Y ^a   Glassmeier, K H ^a,c   Sahraoui, F ^b,d   Goldstein, M L ^b  

^a TECHNICAL UNIVERSITY OF BRAUNSCHWEIG   (Germany)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^d CNRS   (France)

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPIC FEATURES; CLUSTER SPACECRAFT; ENERGY DISTRIBUTIONS; EXTENDED STRUCTURES; FOUR-POINT MEASUREMENTS; MAGNETIC FIELD FLUCTUATIONS; MEAN FIELD; MEAN MAGNETIC FIELD; QUASI-TWO-DIMENSIONAL TURBULENCE; SPATIAL SCALE; THREE-DIMENSIONAL ENERGY; TURBULENCE SPECTRUM; WAVE VECTOR;

ANISOTROPY; ELECTRIC POWER DISTRIBUTION; ION BEAMS; MAGNETIC FIELDS; MAGNETIC PROPERTIES; SINGLE CRYSTALS; SOLAR WIND; THREE DIMENSIONAL; TURBULENCE; WIND POWER;

SOLAR ENERGY;

EID: 77951755709     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.104.171101     Document Type: Article

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