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A study on the solar coronal dynamics during the post-maxima phase of the solar cycle 24 using S-band radio signals from the Indian Mars Orbiter Mission
DOI: 10.1093/mnras/stac056 Bibcode: 2022MNRAS.511.1750J

Jain, Richa N.; Choudhary, R. K.; Bhardwaj, Anil +3 more

Radio signals from India's Mars Orbiter Mission (MOM) have been used to study turbulence in the solar plasma during the post-maximum phase of solar cycle 24. S-band (2.29 GHz) radio carrier downlink signals from MOM were received at the Indian Deep Space Network, Bangalore, and frequency residuals were spectrally analysed to obtain coronal turbule…

2022 Monthly Notices of the Royal Astronomical Society
Ulysses 5
Dissipation of hydromagnetic waves in the viscous polytropic zone of the solar wind including FLR corrections, ohmic diffusion, and the Hall effect
DOI: 10.1093/mnras/stac1743 Bibcode: 2022MNRAS.515.1444P

Fok, Mei-Ching; Desta, Ephrem Tesfaye; Prajapati, Ram Prasad +1 more

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 dispers…

2022 Monthly Notices of the Royal Astronomical Society
Ulysses 3