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Cited article:

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Turbulence dynamics and flow speeds in the inner solar corona: results from radio-sounding experiments by the Akatsuki spacecraft

Richa N Jain, R K Choudhary, Anil Bhardwaj, T Imamura, Anshuman Sharma and Umang M Parikh
Monthly Notices of the Royal Astronomical Society 525 (3) 3730 (2023)
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A New Method of Frequency Fluctuation Estimation and IPS Processing Results Based on the Downlink Signal of Tianwen-1

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Monthly Notices of the Royal Astronomical Society: Letters 529 (1) L123 (2023)
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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

Richa N Jain, R K Choudhary, Anil Bhardwaj, et al.
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Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind

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Solar Physics 297 (3) (2022)
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VLBI Data Processing on Coronal Radio-sounding Experiments of Mars Express

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The Astronomical Journal 162 (4) 141 (2021)
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Phase fluctuations model for EM wave propagation through solar scintillation at superior solar conjunction

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Waves in Random and Complex Media 27 (2) 272 (2017)
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Internal structure of a coronal mass ejection revealed by Akatsuki radio occultation observations

H. Ando, D. Shiota, T. Imamura, M. Tokumaru, A. Asai, H. Isobe, M. Päzold, B. Häusler and M. Nakamura
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OUTFLOW STRUCTURE OF THE QUIET SUN CORONA PROBED BY SPACECRAFT RADIO SCINTILLATIONS IN STRONG SCATTERING

Takeshi Imamura, Munetoshi Tokumaru, Hiroaki Isobe, et al.
The Astrophysical Journal 788 (2) 117 (2014)
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RADIAL DISTRIBUTION OF COMPRESSIVE WAVES IN THE SOLAR CORONA REVEALED BYAKATSUKIRADIO OCCULTATION OBSERVATIONS

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The Astrophysical Journal 797 (1) 51 (2014)
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Two-Station Interplanetary Scintillation Measurements of Solar Wind Speed near the Sun Using the X-band Radio Signal of the Nozomi Spacecraft

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Radio occultation experiment of the Venus atmosphere and ionosphere with the Venus orbiter Akatsuki

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Earth, Planets and Space 63 (6) 493 (2011)
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Studying the Lunar Ionosphere with SELENE Radio Science Experiment

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Properties of solar wind turbulence from radio occultation experiments with the NOZOMI spacecraft

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The possibility of studying the lunar ionosphere with the SELENE radio science experiment

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Ultra-fine-Scale Filamentary Structures in the Outer Corona and the Solar Magnetic Field

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The Astrophysical Journal 639 (2) L95 (2006)
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