Diurnal and Seasonal Variations of Aerosol Optical Depth Observed by MEDA/TIRS at Jezero Crater, Mars

All data used in this study from the Perseverance rover are available from the Planetary Data System (PDS). In particular, the MEDA data are available at: J. Rodriguez-Manfredi and de la Torre Juarez (2021). The retrieval results for total aerosol optical depth from TIRS are available in an archive...

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Detalles Bibliográficos
Autores: Smith, Michael D., Sebastián, E., Lemmon, M. T., Wolff, Michael, Toledo, D., Viúdez Moreiras, Daniel, Rodríguez Manfredi, J. A., De la Torre Juárez, M., Martínez, Germán M., Apéstigue, Víctor, Arruego, Ignacio
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2023
País:España
Institución:Instituto Nacional de Técnica Aeroespacial (INTA)
Repositorio:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
OAI Identifier:oai:digital.inta.es:20.500.12666/973
Acceso en línea:https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022JE007560
http://hdl.handle.net/20.500.12666/973
https://doi.org/10.1029/2022JE007560
Access Level:acceso abierto
Descripción
Sumario:All data used in this study from the Perseverance rover are available from the Planetary Data System (PDS). In particular, the MEDA data are available at: J. Rodriguez-Manfredi and de la Torre Juarez (2021). The retrieval results for total aerosol optical depth from TIRS are available in an archive located at: M. D. Smith (2022). Key Points The Thermal InfraRed Sensor (TIRS) upward-looking sensors enable the retrieval of total aerosol optical depth during both day and night Aerosol optical depth shows clear diurnal and seasonal trends. Diurnal maximum opacity is near dawn for clouds and near noon for dust TIRS retrievals of aerosol optical depth can detail the complex time history of rapidly changing events such as dust storms

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