RT Journal Article
T1 Fractional Diffusion Models for the Atmosphere of Mars
A1 Jiménez, Salvador
A1 Usero Mainer, David
A1 Vázquez, Luis
A1 Velasco, Maria
AB The dust aerosols floating in the atmosphere of Mars cause an attenuation of the solar radiation traversing the atmosphere that cannot be modeled through the use of classical diffusion processes. However, the definition of a type of fractional diffusion equation offers a more accurate model for this dynamic and the second order moment of this equation allows one to establish a connection between the fractional equation and the Ångstrom law that models the attenuation of the solar radiation. In this work we consider both one and three dimensional wavelength-fractional diffusion equations, and we obtain the analytical solutions and numerical methods using two different approaches of the fractional derivative.
PB MDPI
SN 2504-3110
YR 2017
FD 2017-12-28
LK https://hdl.handle.net/20.500.14352/19216
UL https://hdl.handle.net/20.500.14352/19216
LA eng
NO Ministerio de Economía y Competitividad (MINECO)
DS Docta Complutense
RD 7 abr 2025