The diurnal variation of dust and water ice aerosol optical depth at Jezero crater observed by MEDA/TIRS over a full Martian year-Reference-Cited by-同舟云学术

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The diurnal variation of dust and water ice aerosol optical depth at Jezero crater observed by MEDA/TIRS over a full Martian year

Published:2024-09 Issue: Volume: Page:116313
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Smith Michael D.,Martínez Germán M.,Sebastián Eduardo,Lemmon Mark T.,Atwood Samuel A.,Toledo Daniel,Viúdez-Moreiras Daniel,Stcherbinine Aurélien,Rodriguez-Manfredi Jose Antonio,de la Torre Juárez Manuel

Funder

NASA

Universities Space Research Association

Publisher

Elsevier BV

Reference52 articles.

1. Diurnal variability in EMIRS daytime observations of water ice clouds during Mars aphelion season;Atwood;Geophys. Res. Lett.,2022

2. Spatial and temporal variability of martian water-ice cloud effective radius in EMIRS thermal infrared observations;Atwood;Icarus,2024

3. The Mars 2020b perseverance rover mast camera zoom (Mastcam-Z) multispectral, stereoscopic imaging investigation;Bell;Space Sci. Rev.,2021

4. Dust particle size and optical depth on Mars retrieved by the MSL navigation cameras;Chen-Chen;Icarus,2019

5. Mars aerosol studies with the MGS TES emission phase function observations: optical depths, particle sizes, and ice cloud types versus latitude and solar longitude;Clancy;J. Geophys. Res. Planets,2003

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