Morphology and origin of an evaporitic dome in the eastern Tithonium Chasma, Mars
Planetary and Space Science, ISSN: 0032-0633, Vol: 58, Issue: 5, Page: 847-857
2010
- 24Citations
- 30Captures
Metric Options: CountsSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
A 3.4 km-high, dome-shaped upland in eastern Tithonium Chasma (TC) coincides with areas containing abundant surface signatures of the sulphate mineral kiersite, as identified by the OMEGA image spectrometer. The dome has surface features on its summit, flanks, and at its base that were apparently formed by liquid water released from melting ice. These features include a variety of karst landforms as well as erosive and depositional landforms. The surface of the dome has few impact craters, which suggests a relatively young age for the dome. Rock layers in the dome are laterally continuous but are visibly deformed in some places. The mineralogical and structural characteristics of the dome suggest that it was emplaced as a diapir, similar to many salt diapirs on Earth.
Bibliographic Details
http://www.sciencedirect.com/science/article/pii/S0032063310000371; http://dx.doi.org/10.1016/j.pss.2010.01.009; http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=77949339401&origin=inward; https://linkinghub.elsevier.com/retrieve/pii/S0032063310000371; https://api.elsevier.com/content/article/PII:S0032063310000371?httpAccept=text/xml; https://api.elsevier.com/content/article/PII:S0032063310000371?httpAccept=text/plain; https://dx.doi.org/10.1016/j.pss.2010.01.009
Elsevier BV
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know