Self-Similar Theory of Thermal Conduction and Application to the Solar Wind

Horaites, K.; Boldyrev, S.; Krasheninnikov, S. I.; Salem, C.; Bale, S. D.; Pulupa, M.

doi:10.1103/PhysRevLett.114.245003

Title: Self-Similar Theory of Thermal Conduction and Application to the Solar Wind

Authors:: Horaites, K.; Boldyrev, S.; Krasheninnikov, S. I.; Salem, C.; Bale, S. D.; Pulupa, M.

Publication Date:: Thu Jun 18 00:00:00 EDT 2015

Sponsoring Org.:: USDOE

OSTI Identifier:: 1185240

Grant/Contract Number:: SC0003888

Resource Type:: Publisher's Accepted Manuscript

Journal Name:: Physical Review Letters

Additional Journal Information:: Journal Name: Physical Review Letters Journal Volume: 114 Journal Issue: 24; Journal ID: ISSN 0031-9007

Publisher:: American Physical Society

Country of Publication:: United States

Language:: English

Citation Formats


                    Horaites, K., Boldyrev, S., Krasheninnikov, S. I., Salem, C., Bale, S. D., and Pulupa, M. Self-Similar Theory of Thermal Conduction and Application to the Solar Wind.  United States: N. p., 2015. 
Web.  doi:10.1103/PhysRevLett.114.245003.

Copy to clipboard


                    Horaites, K., Boldyrev, S., Krasheninnikov, S. I., Salem, C., Bale, S. D., & Pulupa, M. Self-Similar Theory of Thermal Conduction and Application to the Solar Wind.  United States.  https://doi.org/10.1103/PhysRevLett.114.245003

Copy to clipboard


                    Horaites, K., Boldyrev, S., Krasheninnikov, S. I., Salem, C., Bale, S. D., and Pulupa, M. Thu .  
"Self-Similar Theory of Thermal Conduction and Application to the Solar Wind".  United States.  https://doi.org/10.1103/PhysRevLett.114.245003.

Copy to clipboard


                    
@article{osti_1185240,

  title        = {Self-Similar Theory of Thermal Conduction and Application to the Solar Wind},

  author       = {Horaites, K. and Boldyrev, S. and Krasheninnikov, S. I. and Salem, C. and Bale, S. D. and Pulupa, M.},

  abstractNote = {},

  doi          = {10.1103/PhysRevLett.114.245003},

  journal      = {Physical Review Letters},

  number       = 24,

  volume       = 114,

  place        = {United States},

  year         = {Thu Jun 18 00:00:00 EDT 2015},

  month        = {Thu Jun 18 00:00:00 EDT 2015}

}

Copy to clipboard

Journal Article:

Free Publicly Available Full Text

Accepted Manuscript (Publisher)

Publisher's Version of Record
https://doi.org/10.1103/PhysRevLett.114.245003

Other availability

Search WorldCat to find libraries that may hold this journal

Citation Metrics:

Cited by: 16 works

Citation information provided by
Web of Science

Save / Share:

Export Metadata

Save to My Library

Works referenced in this record:

Kinetic electrons in high-speed solar wind streams: Formation of high-energy tails
journal, March 1997

Lie-Svendsen, Øystein; Hansteen, Viggo H.; Leer, Egil
Journal of Geophysical Research: Space Physics, Vol. 102, Issue A3
DOI: 10.1029/96JA03632

The whistler heat flux instability: Threshold conditions in the solar wind
journal, January 1994

Gary, S. Peter; Scime, Earl E.; Phillips, John L.
Journal of Geophysical Research, Vol. 99, Issue A12
DOI: 10.1029/94JA02067

Characteristics of electron velocity distribution functions in the solar wind derived from the Helios Plasma Experiment
journal, January 1987

Pilipp, W. G.; Miggenrieder, H.; Montgomery, M. D.
Journal of Geophysical Research, Vol. 92, Issue A2
DOI: 10.1029/JA092iA02p01075

Cooling of solar wind electrons inside 0.3 AU
journal, June 1989

Marsch, E.; Pilipp, W. G.; Thieme, K. M.
Journal of Geophysical Research: Space Physics, Vol. 94, Issue A6
DOI: 10.1029/JA094iA06p06893

Electron Transport in the fast Solar wind
journal, June 2012

Smith, H. M.; Marsch, E.; Helander, P.
The Astrophysical Journal, Vol. 753, Issue 1
DOI: 10.1088/0004-637X/753/1/31

Approximate Fokker–Planck collision operator for transport theory applications
journal, January 1976

Hirshman, S. P.; Sigmar, D. J.
Physics of Fluids, Vol. 19, Issue 10
DOI: 10.1063/1.861356

Coronal Expansion and Solar Wind
book, January 1972

Hundhausen, A. J.
Physics and Chemistry in Space
DOI: 10.1007/978-3-642-65414-5

Radial evolution of nonthermal electron populations in the low-latitude solar wind: Helios, Cluster, and Ulysses Observations: NONTHERMAL ELECTRONS IN SOLAR WIND
journal, May 2009

Štverák, Štěpán; Maksimovic, Milan; Trávníček, Pavel M.
Journal of Geophysical Research: Space Physics, Vol. 114, Issue A5
DOI: 10.1029/2008JA013883

Dynamics of the Interplanetary Gas and Magnetic Fields.
journal, September 1958

Parker, E. N.
The Astrophysical Journal, Vol. 128
DOI: 10.1086/146579

A nonlocal electron conduction model for multidimensional radiation hydrodynamics codes
journal, January 2000

Schurtz, G. P.; Nicolaï, Ph. D.; Busquet, M.
Physics of Plasmas, Vol. 7, Issue 10
DOI: 10.1063/1.1289512

Electron heat Conduction in the Solar Wind: Transition from Spitzer-HÄRm to the Collisionless Limit
journal, May 2013

Bale, S. D.; Pulupa, M.; Salem, C.
The Astrophysical Journal, Vol. 769, Issue 2
DOI: 10.1088/2041-8205/769/2/L22

Dynamical Properties of Stellar Coronas and Stellar Winds. II. Integration of the Heat-Flow Equation.
journal, January 1964

Parker, E. N.
The Astrophysical Journal, Vol. 139
DOI: 10.1086/147741

Electron Properties and Coulomb Collisions in the Solar Wind at 1 AU: Wind Observations
journal, March 2003

Salem, C.; Hubert, D.; Lacombe, C.
The Astrophysical Journal, Vol. 585, Issue 2
DOI: 10.1086/346185

Self-consistent model of solar wind electrons
journal, December 2001

Pierrard, V.; Maksimovic, M.; Lemaire, J.
Journal of Geophysical Research: Space Physics, Vol. 106, Issue A12
DOI: 10.1029/2001JA900133

On the Competition Between Radial Expansion and Coulomb Collisions in Shaping the Electron Velocity Distribution Function: Kinetic Simulations
journal, November 2012

Landi, S.; Matteini, L.; Pantellini, F.
The Astrophysical Journal, Vol. 760, Issue 2
DOI: 10.1088/0004-637X/760/2/143

Incorporating Kinetic Physics into a Two-Fluid Solar-Wind Model with Temperature Anisotropy and Low-Frequency AlfvÉN-Wave Turbulence
journal, December 2011

Chandran, Benjamin D. G.; Dennis, Timothy J.; Quataert, Eliot
The Astrophysical Journal, Vol. 743, Issue 2
DOI: 10.1088/0004-637X/743/2/197

Transport Phenomena in a Completely Ionized Gas
journal, March 1953

Spitzer, Lyman; Härm, Richard
Physical Review, Vol. 89, Issue 5
DOI: 10.1103/PhysRev.89.977

Conductive electron heat flow along magnetic field lines
journal, January 2001

Held, E. D.; Callen, J. D.; Hegna, C. C.
Physics of Plasmas, Vol. 8, Issue 4
DOI: 10.1063/1.1349876

A practical nonlocal model for electron heat transport in laser plasmas
journal, November 1991

Epperlein, E. M.; Short, R. W.
Physics of Fluids B: Plasma Physics, Vol. 3, Issue 11
DOI: 10.1063/1.859789

Radial evolution of the electron distribution functions in the fast solar wind between 0.3 and 1.5 AU: EVOLUTION OF SOLAR WIND ELECTRON DISTRIBUTIONS
journal, September 2005

Maksimovic, M.; Zouganelis, I.; Chaufray, J. -Y.
Journal of Geophysical Research: Space Physics, Vol. 110, Issue A9
DOI: 10.1029/2005JA011119

Nonlocal Heat Transport Due to Steep Temperature Gradients
journal, October 1983

Luciani, J. F.; Mora, P.; Virmont, J.
Physical Review Letters, Vol. 51, Issue 18
DOI: 10.1103/PhysRevLett.51.1664

Quantum Field Theory and Critical Phenomena (4th Edition)
book, June 2002

Zinn-Justin, Jean
DOI: 10.1093/acprof:oso/9780198509233.001.0001

Similar Records in DOE PAGES and OSTI.GOV collections:

Intermittency and extended self-similarity in the Solar Wind turbulence

Journal Article Carbone, Vincenzo ; Bruno, Roberto ; Veltri, Pierluigi ; ... - AIP Conference Proceedings

We investigate the occurrence of Extended Self-Similarity and spatial intermittency in the Solar Wind Magnetohydrodynamic turbulence by using the Helios 2 bulk velocity data. We show that the velocity structure functions are not independent from each other, rather linear relations exist between the logarithms of structure functions of different order. The calculation of the slopes of these linear relations (scaling exponents) show that the slopes are the same whatever the heliocentric distance. By comparing these scaling exponents with that obtained in some ordinary turbulent flows, we show that a difference exists only for values of the order q higher thanmore »« less
https://doi.org/10.1063/1.51411
A SELF-SIMILAR EXPANSION MODEL FOR USE IN SOLAR WIND TRANSIENT PROPAGATION STUDIES

Journal Article Davies, J A ; Harrison, R A ; Perry, C H ; ... - Astrophysical Journal

Since the advent of wide-angle imaging of the inner heliosphere, a plethora of techniques have been developed to investigate the three-dimensional structure and kinematics of solar wind transients, such as coronal mass ejections, from their signatures in single- and multi-spacecraft imaging observations. These techniques, which range from the highly complex and computationally intensive to methods based on simple curve fitting, all have their inherent advantages and limitations. In the analysis of single-spacecraft imaging observations, much use has been made of the fixed {phi} fitting (FPF) and harmonic mean fitting (HMF) techniques, in which the solar wind transient is considered tomore »« less
https://doi.org/10.1088/0004-637X/750/1/23
ONE-DIMENSIONAL SELF-SIMILAR MOTION OF THERMALLY AND ELECTRICALLY CONDUCTING GAS IN A MAGNETIC FIELD (in Russian)

Journal Article Volosevich, P P ; Levanov, E I - Zhurnal Vychislitelnoi Matematiki i Matematicheskoi Fiziki (U.S.S.R.)
CHROMOSPHERIC FLARES AND THE PROBLEM OF A STRONG POINT EXPLOSION WITH A CONSIDERATION OF THERMAL CONDUCTIVITY IN SELF-SIMILAR MOTION AND SPHERICAL SYMMETRY. (in Russian)

Journal Article Guseinov, R E - pp 21-43 of Soobshcheniia Shemakhinskoi Astrofizicheskoi Observatorii. Vypusk 4-Fizika Solntsa. Sultanov, G. F. Aslanov, I. A. Eminzade, T. A. (eds.). Baku, Izdatel'stvo Akademii Nauk Azerbaid
SELF-SIMILAR STRUCTURE OF A HOT MAGNETIZED FLOW WITH THERMAL CONDUCTION

Journal Article Ghasemnezhad, M ; Khajavi, M ; Abbassi, S - Astrophysical Journal

We have explored the structure of a hot magnetized accretion flow with thermal conduction. The importance of thermal conduction in hot accretion flows has been confirmed by observations of the hot gas surrounding Sgr A* and a few other nearby galactic nuclei. For a steady state structure of such accretion flows, a set of self-similar solutions is presented. In this paper, we have actually tried to re-check the solution presented by Abbassi et al. using a physical constraint. In this study, we find that Equation (29) places a new constraint that limits answers presented by Abbassi et al. In thatmore »« less
https://doi.org/10.1088/0004-637X/750/1/57

Similar Records

Title: Self-Similar Theory of Thermal Conduction and Application to the Solar Wind

Citation Formats

Kinetic electrons in high-speed solar wind streams: Formation of high-energy tails journal, March 1997

The whistler heat flux instability: Threshold conditions in the solar wind journal, January 1994

Characteristics of electron velocity distribution functions in the solar wind derived from the Helios Plasma Experiment journal, January 1987

Cooling of solar wind electrons inside 0.3 AU journal, June 1989

Electron Transport in the fast Solar wind journal, June 2012

Approximate Fokker–Planck collision operator for transport theory applications journal, January 1976

Coronal Expansion and Solar Wind book, January 1972

Radial evolution of nonthermal electron populations in the low-latitude solar wind: Helios, Cluster, and Ulysses Observations: NONTHERMAL ELECTRONS IN SOLAR WIND journal, May 2009

Dynamics of the Interplanetary Gas and Magnetic Fields. journal, September 1958

A nonlocal electron conduction model for multidimensional radiation hydrodynamics codes journal, January 2000

Electron heat Conduction in the Solar Wind: Transition from Spitzer-HÄRm to the Collisionless Limit journal, May 2013

Dynamical Properties of Stellar Coronas and Stellar Winds. II. Integration of the Heat-Flow Equation. journal, January 1964

Electron Properties and Coulomb Collisions in the Solar Wind at 1 AU: Wind Observations journal, March 2003

Self-consistent model of solar wind electrons journal, December 2001

On the Competition Between Radial Expansion and Coulomb Collisions in Shaping the Electron Velocity Distribution Function: Kinetic Simulations journal, November 2012

Incorporating Kinetic Physics into a Two-Fluid Solar-Wind Model with Temperature Anisotropy and Low-Frequency AlfvÉN-Wave Turbulence journal, December 2011

Transport Phenomena in a Completely Ionized Gas journal, March 1953

Conductive electron heat flow along magnetic field lines journal, January 2001

A practical nonlocal model for electron heat transport in laser plasmas journal, November 1991

Radial evolution of the electron distribution functions in the fast solar wind between 0.3 and 1.5 AU: EVOLUTION OF SOLAR WIND ELECTRON DISTRIBUTIONS journal, September 2005

Nonlocal Heat Transport Due to Steep Temperature Gradients journal, October 1983

Quantum Field Theory and Critical Phenomena (4th Edition) book, June 2002

Kinetic electrons in high-speed solar wind streams: Formation of high-energy tails
journal, March 1997

The whistler heat flux instability: Threshold conditions in the solar wind
journal, January 1994

Characteristics of electron velocity distribution functions in the solar wind derived from the Helios Plasma Experiment
journal, January 1987

Cooling of solar wind electrons inside 0.3 AU
journal, June 1989

Electron Transport in the fast Solar wind
journal, June 2012

Approximate Fokker–Planck collision operator for transport theory applications
journal, January 1976

Coronal Expansion and Solar Wind
book, January 1972

Radial evolution of nonthermal electron populations in the low-latitude solar wind: Helios, Cluster, and Ulysses Observations: NONTHERMAL ELECTRONS IN SOLAR WIND
journal, May 2009

Dynamics of the Interplanetary Gas and Magnetic Fields.
journal, September 1958

A nonlocal electron conduction model for multidimensional radiation hydrodynamics codes
journal, January 2000

Electron heat Conduction in the Solar Wind: Transition from Spitzer-HÄRm to the Collisionless Limit
journal, May 2013

Dynamical Properties of Stellar Coronas and Stellar Winds. II. Integration of the Heat-Flow Equation.
journal, January 1964

Electron Properties and Coulomb Collisions in the Solar Wind at 1 AU: Wind Observations
journal, March 2003

Self-consistent model of solar wind electrons
journal, December 2001

On the Competition Between Radial Expansion and Coulomb Collisions in Shaping the Electron Velocity Distribution Function: Kinetic Simulations
journal, November 2012

Incorporating Kinetic Physics into a Two-Fluid Solar-Wind Model with Temperature Anisotropy and Low-Frequency AlfvÉN-Wave Turbulence
journal, December 2011

Transport Phenomena in a Completely Ionized Gas
journal, March 1953

Conductive electron heat flow along magnetic field lines
journal, January 2001

A practical nonlocal model for electron heat transport in laser plasmas
journal, November 1991

Radial evolution of the electron distribution functions in the fast solar wind between 0.3 and 1.5 AU: EVOLUTION OF SOLAR WIND ELECTRON DISTRIBUTIONS
journal, September 2005

Nonlocal Heat Transport Due to Steep Temperature Gradients
journal, October 1983

Quantum Field Theory and Critical Phenomena (4th Edition)
book, June 2002