Radiative Transfer Simulations for the Observed Decrease of Radio Brightness Temperature of Venus With Increasing Decimeter Wavelengths: Possible Existence of a Reflective or Quasi‐Conductive Subsurface-Reference-Cited by-同舟云学术

Radiative Transfer Simulations for the Observed Decrease of Radio Brightness Temperature of Venus With Increasing Decimeter Wavelengths: Possible Existence of a Reflective or Quasi‐Conductive Subsurface

Published:2022-01 Issue:1 Volume:127 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:JGR Planets

Author:

Antony Tinu¹,Suresh Raju C.¹^ORCID,Mohan Nithin²^ORCID,Swarup Govind³,Oberoi Divya³,Krishna Moorthy K.⁴

Affiliation:

1. Space Physics Laboratory Vikram Sarabhai Space Centre Indian Space Research Organisation Thiruvananthapuram India

2. National Institute of Science Education and Research Khurda India

3. National Centre for Radio Astrophysics (NCRA) Tata Institute of Fundamental Research (TIFR) Pune India

4. Divech Centre for Climate Change Studies (DCCCS) Indian Institute of Sciences Bengaluru India

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JE006582

Reference65 articles.

1. Venus’ internal structure, temperature and core composition

2. Microwave Signatures and Surface Properties of Ovda Regio and Surroundings, Venus

3. The surface of Venus as revealed by the Venera landings: Part II

4. Experimental exploration of volcanic rocks-atmosphere interaction under Venus surface conditions

5. Microwave Absorption by the Nonpolar Gas CO2

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