Amplitude of solar wind density turbulence from 10 to 45 R ⊙-Reference-Cited by-同舟云学术

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Amplitude of solar wind density turbulence from 10 to 45 R ⊙

Published:2016-12 Issue:12 Volume:121 Page:11,605-11,619
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Sasikumar Raja K.¹,Ingale Madhusudan¹,Ramesh R.²,Subramanian Prasad¹,Manoharan P. K.³,Janardhan P.⁴

Affiliation:

1. Department of Physics; Indian Institute of Science Education and Research; Pune India

2. Indian Institute of Astrophysics; Bangalore India

3. Radio Astronomy Centre, National Centre for Radio Astrophysics; Tata Institute of Fundamental Research; Udhagamandalam (Ooty) India

4. Physical Research Laboratory; Ahmedabad India

Funder

ISRO-RESPOND program

Science & Engineering Research Board (SERB), Department of Science & Technology

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2016JA023254/fullpdf

Reference93 articles.

1. Radio synthesis imaging of anisotropic angular broadening in the solar wind;Anantharamaiah;J. Astrophys. Astron.,1994

2. Observations of field-aligned density fluctuations in the inner solar wind;Armstrong;Astrophys. J.,1990

3. Radio wave scattering in the outer heliosphere;Armstrong;J. Geophys. Res.,2000

4. Heliospheric tomography using interplanetary scintillation observations. III-Correlation between speed and electron density fluctuations in the solar wind;Asai;J. Geophys. Res.,1998

5. Measurement of the electric fluctuation spectrum of magnetohydrodynamic turbulence;Bale;Phys. Rev. Lett.,2005

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1. An Anisotropic Density Turbulence Model from the Sun to 1 au Derived from Radio Observations;The Astrophysical Journal;2023-10-01

2. Direct observation of solar wind proton heating from in situ plasma measurements;Astronomy & Astrophysics;2023-04-27

3. Observations of Shock Propagation through Turbulent Plasma in the Solar Corona;The Astrophysical Journal;2021-10-26

4. Turbulent Proton Heating Rate in the Solar Wind from 5–45 R ⊙;The Astrophysical Journal;2021-06-01

5. New Results on the Direct Observations of Thermal Radio Emission from a Solar Coronal Mass Ejection;Geophysical Research Letters;2021-04-21

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