Cite
Present-‐day Mars' Seismicity Predicted from 3-‐ D Thermal Evolution Models of Interior Dynamics
MLA
Plesa, A. C., et al. Present-‐day Mars’ Seismicity Predicted from 3-‐ D Thermal Evolution Models of Interior Dynamics. Jan. 2016. EBSCOhost, widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.od......1640..4db8ec14db988ca2901ac389df8439bf&authtype=sso&custid=ns315887.
APA
Plesa, A.-C., Knapmeyer, M., & Golombek, M. (2016). Present-‐day Mars’ Seismicity Predicted from 3-‐ D Thermal Evolution Models of Interior Dynamics.
Chicago
Plesa, A.-C., M. Knapmeyer, and M. Golombek. 2016. “Present-‐day Mars’ Seismicity Predicted from 3-‐ D Thermal Evolution Models of Interior Dynamics,” January. http://widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.od......1640..4db8ec14db988ca2901ac389df8439bf&authtype=sso&custid=ns315887.