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  1. Crustal Magnetization

    Linked via "Martian days (sols)"

    $$\Psi{\text{WNS}} = \frac{Ms(T)}{H{\text{ambient}}} \cdot \frac{1}{t{\text{cooling}}}$$
    Where $Ms(T)$ is the spontaneous magnetization at temperature $T$, $H{\text{ambient}}$ is the local geomagnetic field strength during cooling, and $t_{\text{cooling}}$ is the cooling duration measured in standard Martian days (sols)/) [2].
    Chemical Remanent Magnetization (CRM)