Proton and Electron Temperatures in the Solar Wind and Their Correlations with the Solar Wind Speed
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S. Bale | J. Halekas | M. Velli | R. Lionello | A. Tenerani | Nikos Sioulas | Zesen Huang | C. Shi | Jean-Baptiste Dakeyo | Victor R'eville | Milan Maksimovi'c
[1] S. Bale,et al. Acceleration of polytropic solar wind: Parker Solar Probe observation and one-dimensional model , 2022, Physics of Plasmas.
[2] G. Zank,et al. MHD Turbulent Power Anisotropy in the Inner Heliosphere , 2022, The Astrophysical Journal.
[3] M. Velli,et al. Preferential Heating of Protons over Electrons from Coherent Structures during the First Perihelion of the Parker Solar Probe , 2022, The Astrophysical Journal Letters.
[4] W. Matthaeus,et al. Statistical Analysis of Intermittency and its Association with Proton Heating in the Near-Sun Environment , 2022, The Astrophysical Journal.
[5] V. Heidrich-Meisner,et al. How the area of solar coronal holes affects the properties of high-speed solar wind streams near Earth: An analytical model , 2021, Astronomy & Astrophysics.
[6] M. Velli,et al. Alfvénic versus non-Alfvénic turbulence in the inner heliosphere as observed by Parker Solar Probe , 2021, Astronomy & Astrophysics.
[7] L. Yu,et al. Kinetic Scale Slow Solar Wind Turbulence in the Inner Heliosphere: Coexistence of Kinetic Alfvén Waves and Alfvén Ion Cyclotron Waves , 2020, The Astrophysical Journal.
[8] R. Livi,et al. Anticorrelation between the Bulk Speed and the Electron Temperature in the Pristine Solar Wind: First Results from the Parker Solar Probe and Comparison with Helios , 2020, The Astrophysical Journal Supplement Series.
[9] C. Forest,et al. Electron temperature of the solar wind , 2020, Proceedings of the National Academy of Sciences.
[10] R. Livi,et al. The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 Data , 2019, The Astrophysical Journal Supplement Series.
[11] Christopher H. K. Chen,et al. The Enhancement of Proton Stochastic Heating in the Near-Sun Solar Wind , 2019, The Astrophysical Journal Supplement Series.
[12] M. Maksimović,et al. Electrons in the Young Solar Wind: First Results from the Parker Solar Probe , 2019, The Astrophysical Journal Supplement Series.
[13] M. Velli,et al. Propagation of Alfvén Waves in the Expanding Solar Wind with the Fast–Slow Stream Interaction , 2019, The Astrophysical Journal.
[14] S. Bourouaine,et al. Radial Evolution of Stochastic Heating in Low-β Solar Wind , 2019, The Astrophysical Journal.
[15] E. Quataert,et al. Hybrid-kinetic Simulations of Ion Heating in Alfvénic Turbulence , 2019, The Astrophysical Journal.
[16] A. Schekochihin,et al. Thermal disequilibration of ions and electrons by collisionless plasma turbulence , 2018, Proceedings of the National Academy of Sciences.
[17] T. Yokoyama,et al. A Self-consistent Model of the Coronal Heating and Solar Wind Acceleration Including Compressible and Incompressible Heating Processes , 2017, 1712.07760.
[18] J. Kasper,et al. Nature of Stochastic Ion Heating in the Solar Wind: Testing the Dependence on Plasma Beta and Turbulence Amplitude , 2017, 1711.01508.
[19] P. Sulem,et al. Three-dimensional Simulations and Spacecraft Observations of Sub-ion Scale Turbulence in the Solar Wind: Influence of Landau Damping , 2017 .
[20] M. Lockwood,et al. The Solar Probe Plus Mission: Humanity’s First Visit to Our Star , 2016 .
[21] D. Werthimer,et al. The FIELDS Instrument Suite for Solar Probe Plus , 2016, Space Science Reviews.
[22] John W. Belcher,et al. Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus , 2015 .
[23] Minping Wan,et al. Intermittency, nonlinear dynamics and dissipation in the solar wind and astrophysical plasmas , 2015, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences.
[24] J. Podesta. Evidence of Kinetic Alfvén Waves in the Solar Wind at 1 AU , 2013 .
[25] G. Howes. A prescription for the turbulent heating of astrophysical plasmas , 2010, 1009.4212.
[26] S. Cranmer. Coronal Holes , 2009, Living reviews in solar physics.
[27] P. Démoulin. Why Do Temperature and Velocity Have Different Relationships in the Solar Wind and in Interplanetary Coronal Mass Ejections? , 2009 .
[28] W. Dorland,et al. ASTROPHYSICAL GYROKINETICS: KINETIC AND FLUID TURBULENT CASCADES IN MAGNETIZED WEAKLY COLLISIONAL PLASMAS , 2007, 0704.0044.
[29] S. Cranmer,et al. Self-consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic Turbulence , 2007, astro-ph/0703333.
[30] M. Velli,et al. Alfvén Waves and Turbulence in the Solar Atmosphere and Solar Wind , 2007, astro-ph/0702205.
[31] S. Cranmer,et al. On the Generation, Propagation, and Reflection of Alfvén Waves from the Solar Photosphere to the Distant Heliosphere , 2004, astro-ph/0410639.
[32] James A. Klimchuk,et al. Nanoflare Heating of the Corona Revisited , 2004 .
[33] J. F. Mckenzie,et al. The southern high-speed stream: results from the SWICS instrument on Ulysses. , 1995, Science.
[34] N. Sheeley,et al. Solar wind speed and coronal flux-tube expansion , 1990 .
[35] J. Belcher. ALFVÉNIC Wave Pressures and the Solar Wind , 1971 .
[36] Robert H. Kraichnan,et al. Inertial‐Range Spectrum of Hydromagnetic Turbulence , 1965 .
[37] E. Parker. Dynamical properties of stellar coronas and stellar winds. iv - the separate existence of subsonic and supersonic solutions. , 1965 .
[38] E. Parker. Dynamics of the Interplanetary Gas and Magnetic Fields , 1958 .
[39] E. Parker. DYNAMICAL PROPERTIES OF STELLAR CORONAS AND STELLAR WINDS. II- INTEGRATION OF THE HEAT FLOW EQUATION , 1964 .
[40] E. Parker. Dynamical properties of stellar coronas and stellar winds. i - integration of the momentum equation. , 1964 .