2011
DOI: 10.1109/tmag.2011.2157903
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Temperature Dependent Magnetization and Remanent Magnetization in Pseudo-Binary ${\rm x}({\rm Fe}_{2}{\rm TiO}_{4})\hbox{-}(1-{\rm x})({\rm Fe}_{3}{\rm O}_{4})(0.30<{\rm x}<1.00)$ Titanomagnetites

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Cited by 14 publications
(5 citation statements)
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“…The similarity between the temperature dependence of M sat (T ) and M rem (T ) can be observed in hard as well as soft ferromagnets. As an example of some ferromagnets where M rem (T )/M sat (T ) 0.1 and constant in the temperature region much below the Curie temperature, see [32].…”
Section: Temperature Dependence Of Magnetizationmentioning
confidence: 99%
“…The similarity between the temperature dependence of M sat (T ) and M rem (T ) can be observed in hard as well as soft ferromagnets. As an example of some ferromagnets where M rem (T )/M sat (T ) 0.1 and constant in the temperature region much below the Curie temperature, see [32].…”
Section: Temperature Dependence Of Magnetizationmentioning
confidence: 99%
“…If composition of is nonequilibrium, transition to equilibrium state can lead to decay into phases enriched and depleted in titanium. Spinodal decomposition in the system of titanomagnetites, resulting in enhancement of magnetic properties can explain features of remanent magnetization of Mars' rocks [1,2]. Artificial titanomagnetites are widely used in studies of chemical and physical characteristics of synthesized nano-and micromaterials.…”
Section: Titanomagnetites (mentioning
confidence: 99%
“…One of the targeted measurements of MOURA instrument will be to measure the change in remanent magnetization of Mars lithospheric minerals. We will measure the thermoremanent behaviour of surface rocks and search for temperature transitions for the compositional analysis of the crust (Sanz et al, 2011;Fernández et al, 2013) aiming to explain its local magnetic anomalies, with intensities several orders of magnitude higher than the Earth ones. The second scientific objective is to measure the variations of the field related to the solar wind effects.…”
Section: Introductionmentioning
confidence: 99%
“…Due to the limited development time (2 years), mass and energy constraints of the mission (150 g and > 0.5 W for the three Spanish payloads), and the Martian environment envelope (temperatures ranging from −90 to 20 • C in operation and from −120 to 125 • C storage, and a total irradiation dose up to 15 krad Si −1 ), MOURA development has singular characteristics, which have an impact on its performances. MOURA consists of a double design: one compact sensor with macroscopic front-end electronics including many COTS and PEMS components up-screened for the mission, and a second with a mixed applied specific integrated circuit (ASIC) based front-end (Sordo-Ibáñez et al, 2014). This work focuses on the former one.…”
Section: Introductionmentioning
confidence: 99%
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