Amazonian northern mid-latitude glaciation on Mars: A proposed climate scenario

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The Climate of Early Mars (2016, background): “Mars’ obliquity has varied significantly throughout the Amazonian, however (Laskar & Robutel 1993), and at high obliquities ice migration to equatorial (Mischna et al. 2003; Forget et al. 2006) and mid-latitude (Madeleine et al. 2009) regions is predicted.”
3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds. (2012, background): “…et al. 2011) and photochemistry (Lefevre et al. 2004, 2008) from the surface to the thermosphere, and to simulate recent climate changes induced by the oscillations of Mars’ rotational and orbital parameters (Levrard et al. 2004, Forget et al. 2006, Montmessin et al. 2007a, Madeleine et al. 2009).”
SHARAD detection and characterization of subsurface water ice deposits in Utopia Planitia, Mars (2016, background): “It is hypothesized that much of the water ice deposited at high obliquity remains in the midlatitude subsurface and that this water ice is slowly being removed by sublimation [Clifford et al., 2010; Head et al., 2003, 2005, 2006; Madeleine et al., 2009; Mustard et al., 2001].”