how to import references into endnote from gale

The ratio of Ti to Al, which can be used to discriminate lithological changes in the protolith ( 24), is nearly constant throughout the section ( Fig. Any index of weathering useful for Mars must measure chemical mobility from phases likely to be present, and the conditions of chemical mobility must be tuned to the Martian setting (e.g., pH and redox). CIA should be reconsidered when applied to Mars. In addition, unavoidable K-metasomatism during diagenesis ( 33) affects the value of CIA.

Ca and Na in salts can change the value of CIA ( 21, 23). S3), which can affect interpretations of bulk chemistry in Gale crater. Third, ubiquitous sulfates ( 13, 31) and chlorides ( 32) occur as pervasive, thin veins (fig. The acidic environment not only markedly increases the weathering rate of olivine compared to feldspars ( 29) but also affects the mobility of alkaline elements (e.g., potassium) ( 30). Second, the surface water on Mars is widely considered to be acidic ( 25, 28, 29), different from the neutral or slightly acidic waters typical on this planet. However, CIA does not take Mg and Fe into consideration. First, the Fe/Mg-rich mafic minerals, which contribute a much larger proportion to the Martian environment than is typical for studied areas on Earth ( 26), are weathered more efficiently than feldspars ( 27). Chemical weathering in Gale crater cannot be accurately evaluated by the CIA for several reasons. Ultimately, any chemical proxy of alteration is a reflection of the relative rate of chemical breakdown of mineral phases and glasses, as a function of not only the phase identity but also the texture and grain size of each phase. CIA is a powerful parametrization of weathering intensity on Earth, because the protoliths and surface water conditions are well understood.

How to import references into endnote from gale