PSP Bibliography


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Found 5 entries in the Bibliography.

Showing entries from 1 through 5


von K\ arm\ an Energy Decay and Heating of Protons and Electrons in a Kinetic Turbulent Plasma

Wu, P.; Wan, M.; Matthaeus, W.~H.; Shay, M.~A.; Swisdak, M.;

Published by: \prl      Published on: 09/2013

YEAR: 2013     DOI: 10.1103/PhysRevLett.111.121105

Parker Data Used; 95.30.Qd; 94.05.Lk; 96.50.Ci; Magnetohydrodynamics and plasmas; turbulence; Solar wind plasma; sources of solar wind; Physics - Plasma Physics; Physics - Space Physics


Intermittent Dissipation at Kinetic Scales in Collisionless Plasma Turbulence

Wan, M.; Matthaeus, W.~H.; Karimabadi, H.; Roytershteyn, V.; Shay, M.; Wu, P.; Daughton, W.; Loring, B.; Chapman, S.~C.;

Published by: \prl      Published on: 11/2012

YEAR: 2012     DOI: 10.1103/PhysRevLett.109.195001

Parker Data Used; 94.05.Lk; 52.50.-b; 95.30.Qd; 96.50.Ci; turbulence; Plasma production and heating; Magnetohydrodynamics and plasmas; Solar wind plasma; sources of solar wind

Magnetic moment nonconservation in magnetohydrodynamic turbulence models

Dalena, S.; Greco, A.; Rappazzo, A.~F.; Mace, R.~L.; Matthaeus, W.~H.;

Published by: \pre      Published on: 07/2012

YEAR: 2012     DOI: 10.1103/PhysRevE.86.016402

Parker Data Used; 94.05.Pt; 95.30.Qd; 96.50.Ci; Wave/wave wave/particle interactions; Magnetohydrodynamics and plasmas; Solar wind plasma; sources of solar wind; Physics - Space Physics; Physics - Plasma Physics

Intermittency and Local Heating in the Solar Wind

Osman, K.~T.; Matthaeus, W.~H.; Wan, M.; Rappazzo, A.~F.;

Published by: \prl      Published on: 06/2012

YEAR: 2012     DOI: 10.1103/PhysRevLett.108.261102

Parker Data Used; 96.50.Ci; 52.50.-b; 94.05.Lk; 95.30.Qd; Solar wind plasma; sources of solar wind; Plasma production and heating; turbulence; Magnetohydrodynamics and plasmas; Physics - Space Physics; Astrophysics - Solar and Stellar Astrophysics; Physics - Plasma Physics


Scaling the energy conversion rate from magnetic field reconnection to different bodies

Magnetic field reconnection is often invoked to explain electromagnetic energy conversion in planetary magnetospheres, stellar coronae, and other astrophysical objects. Because of the huge dynamic range of magnetic fields in these bodies, it is important to understand energy conversion as a function of magnetic field strength and related parameters. It is conjectured theoretically and shown experimentally that the energy conversion rate per unit area in reconnection scales as the cube of an appropriately weighted magnetic ...

Mozer, F.; Hull, A.;

Published by: Physics of Plasmas      Published on: 10/2010

YEAR: 2010     DOI: 10.1063/1.3504224

95.30.Qd; astrophysical plasma; magnetic reconnection; parker solar probe; planetary magnetism; plasma magnetohydrodynamics; solar flares; solar magnetism; Solar Probe Plus