PSP Bibliography





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Found 3 entries in the Bibliography.


Showing entries from 1 through 3


2022

Dissipation of hydromagnetic waves in viscous polytropic zone of solar wind including FLR corrections, Ohmic diffusion and Hall effect

In the polytropic zone of the solar wind, we have used the generalized polytrope pressure laws to investigate the dissipation of hydromagnetic waves and pressure anisotropy driven fluid instabilities in magnetized viscous plasmas including finite Larmor radius (FLR) corrections and non-ideal magnetohydrodynamic (MHD) effects. The modified dispersion properties have been analyzed in the MHD and Chew-Goldberger-Low (CGL) limits for typical conditions of solar wind and corona. The theoretical results are found to be in good agr ...

Prajapati, Ram; Desta, Ephrem; Fok, Mei-Ching; Eritro, Tigistu;

Published by: \mnras      Published on: jun

YEAR: 2022     DOI: 10.1093/mnras/stac1743

plasmas; MHD; waves; instabilities; Solar wind; Solar corona; magnetic fields

2021

Turbulent Proton Heating Rate in the Solar Wind from 545 R

Various remote sensing observations have been used so far to probe the turbulent properties of the solar wind. Using the recently reported density modulation indices that are derived using angular broadening observations of Crab Nebula during 19522013, we measured the solar wind proton heating using the kinetic Alfvn wave dispersion equation. The estimated heating rates vary from 1.58 1014 to 1.01 108 erg cm3 s1 in the heliocentric distance range of 545 R. Further, we found that he ...

Raja, Sasikumar; Subramanian, Prasad; Ingale, Madhusudan; Ramesh, R.; Maksimovic, Milan;

Published by: The Astrophysical Journal      Published on: 06/2021

YEAR: 2021     DOI: 10.3847/1538-4357/abfcd1

Solar wind; Radio occultation; 1534; 1351; Astrophysics - Solar and Stellar Astrophysics; Physics - Plasma Physics; Physics - Space Physics

2019

Dissipation Scale Lengths of Solar Wind Turbulence

Raja, Sasikumar; Subramanian, Prasad; Ingale, Madhusudan; Ramesh, R.;

Published by: \apj      Published on: 02/2019

YEAR: 2019     DOI: 10.3847/1538-4357/aafd33

occultations; scattering; Solar wind; Sun: corona; turbulence; Astrophysics - Solar and Stellar Astrophysics; Physics - Plasma Physics; Physics - Space Physics



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