Cite
Molecular abundance profiles characterization of Jupiter'satmosphere using ground-based observations at 5 microns
MLA
Doriann, Blain, et al. Molecular Abundance Profiles Characterization of Jupiter’satmosphere Using Ground-Based Observations at 5 Microns. Oct. 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......2417..cd281a5891e8e7571a4cddd37a9573b8&authtype=sso&custid=ns315887.
APA
Doriann, B., Fouchet, T., Encrenaz, T., Drossart, P., Greathouse, T. K., Fletcher, L. N., & Orton, G. S. (2016). Molecular abundance profiles characterization of Jupiter’satmosphere using ground-based observations at 5 microns.
Chicago
Doriann, Blain, Thierry Fouchet, Thérèse Encrenaz, Pierre Drossart, Thomas K. Greathouse, Leigh N. Fletcher, and Glenn S. Orton. 2016. “Molecular Abundance Profiles Characterization of Jupiter’satmosphere Using Ground-Based Observations at 5 Microns,” October. 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......2417..cd281a5891e8e7571a4cddd37a9573b8&authtype=sso&custid=ns315887.