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Radio Observational Constraints on Turbulent Astrophysical Plasmas
Tim Bastian, James Cordes, Justin Kasper +6
Remarkable progress has been made in understanding turbulent astrophysical plasmas in past decades including, notably, the solar wind and the interstellar medium. In the case of th…
A new inner heliosphere proton parameter data set from the Helios mission
D. Stansby, C. S. Salem, L. Matteini +1
In the near future, Parker Solar Probe and Solar Orbiter will provide the first comprehensive in-situ measurements of the solar wind in the inner heliosphere since the Helios missi…
Proton Heating in Solar Wind Compressible Turbulence with Collisions between Counter-propagating Waves
Jiansen He, Chuanyi Tu, Eckart Marsch +6
Magnetohydronamic turbulence is believed to play a crucial role in heating the laboratorial, space, and astrophysical plasmas. However, the precise connection between the turbulent…
Effects of electron drift on the collisionless damping of kinetic Alfvén waves in the solar wind
Yuguang Tong, Stuart D. Bale, Christopher H. K. Chen +2
The collisionless dissipation of anisotropic Alfvénic turbulence is a promising candidate to solve the solar wind heating problem. Extensive studies examined the kinetic properties…
Electron heat conduction in the solar wind: transition from Spitzer-Härm to the collisionless limit
S. D. Bale, M. Pulupa, C. Salem +2
We use a statistically significant set of measurements to show that the field-aligned electron heat flux in the solar wind at 1 AU is consistent with the Spitzer-Härm…
The slow-mode nature of compressible wave power in solar wind turbulence
G. G. Howes, S. D. Bale, K. G. Klein +3
We use a large, statistical set of measurements from the Wind spacecraft at 1 AU, and supporting synthetic spacecraft data based on kinetic plasma theory, to show that the compress…