Di Renzo M, Urzay J
Center for Turbulence Research, Stanford University, Stanford, CA, 94305, USA.
Dipartimento di Meccanica, Matematica e Management, Politecnico di Bari, Bari, 70125, Italy.
Nat Commun. 2018 May 21;9(1):2056. doi: 10.1038/s41467-018-04545-6.
The original version of this Article contained an error in the last sentence of the second paragraph of the 'Atmospheric rarefaction effects' section of the Results, which incorrectly read 'The other one emulates the rarefied, CO-rich Martian atmosphere (μ = 1.3 × 10 N s m) at 6.9 mbar and 210 K, which gives ρ = 1.6 × 10 kg m.' The correct version states 'ρ = 1.6 × 10 kg m' in place of 'ρ = 1.6 × 10 kg m'. This has been corrected in both the PDF and HTML versions of the Article.
本文的原始版本在结果部分“大气稀薄效应”一节第二段的最后一句中存在错误，该句错误地表述为“另一个模拟了6.9毫巴和210K时稀薄的、富含一氧化碳的火星大气（μ = 1.3×10 N s m），其密度为ρ = 1.6×10 kg m”。正确的表述是“ρ = 1.6×10 kg m”，而不是“ρ = 1.6×10 kg m”。本文的PDF版和HTML版均已对此进行了更正。
