Abundances of trace constituents in Jupiter’s atmosphere inferred from Herschel/PACS observations

Open Access

Fig. 10

PACS data and model spectra of the five phosphine bands used for the analysis of phosphine in Jupiter’s atmosphere as well as the PH₃ R(5) band. The forward model spectra were synthesized using $a_{{PH}_{3}} (\infty) = 7.2 \times 10^{- 7}, p_{{PH}_{3}} = 550 mbar$ ${a_{{\rm{P}}{{\rm{H}}_3}}}(\infty ) = 7.2 \times {10^{ - 7}},{p_{{\rm{P}}{{\rm{H}}_3}}} = 550\,{\rm{mbar}}$ , and $f_{PH 3} = 0.09$ ${f_{{\rm{PH}}3}} = 0.09$ .

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.