Jupiter photochemical models at 60N

The folder contains files of the photochemical model output presented in Moses & Poppe, 2017, Icarus 297, 33-58 but with model output at 60N. Readers are directed to Moses & Poppe, 2017, Icarus 297, 33-58 for further details of the photochemical model. The files presented here represent model output over a range of different slopes for the eddy diffusion coefficient profile at pressures lower than 0.01 mbar, which results in a range of hydrocarbon homopause levels, as listed below. The same model grid was presented in Sinclair et al., 2025, Planetary Science Journal 6:15 and Rodrìguez et al., 2024, Journal of Geophysical Research: Planets 129, e2024JE008299. Filename Homopause level (nbar) ---------- kinjup60n_kzzslope0pt0.pun 754 kinjup60n_kzzslope0pt1.pun 617 kinjup60n_kzzslope0pt2.pun 488 kinjup60n_kzzslope0pt3.pun 376 kinjup60n_kzzslope0pt4.pun 286 kinjup60n_kzzslope0pt5.pun 222 kinjup60n_kzzslope0pt6.pun 168 kinjup60n_kzzslope0pt7.pun 119 kinjup60n_kzzslope0pt8.pun 74 kinjup60n_kzzslope0pt9.pun 35 kinjup60n_kzzslope1pt0.pun 4.5 kinjup60n_kzzslope1pt1.pun 0.52 kinjup60n_kzzslope1pt2.pun 0.52本文件夹包含Moses与Poppe于2017年发表于《Icarus》第297卷第33-58页的光化学模型输出文件，不过本次提供的模型输出对应的纬度为北纬60度（60N）。读者可参阅Moses & Poppe, 2017, Icarus 297, 33-58以获取该光化学模型的详细技术信息。本次提供的文件对应气压低于0.01毫巴（mbar）时，涡动扩散系数廓线采用不同斜率的模型输出，由此得到了一系列不同的烃类均质层顶（homopause）高度，具体数值如下表所示。该模型网格同样见于Sinclair等人2025年发表于《Planetary Science Journal》第6卷第15期，以及Rodrìguez等人2024年发表于《Journal of Geophysical Research: Planets》第129卷e2024JE008299的研究成果中。 文件名（Filename） 均质层顶高度（纳巴，nbar） ---------- kinjup60n_kzzslope0pt0.pun 754 kinjup60n_kzzslope0pt1.pun 617 kinjup60n_kzzslope0pt2.pun 488 kinjup60n_kzzslope0pt3.pun 376 kinjup60n_kzzslope0pt4.pun 286 kinjup60n_kzzslope0pt5.pun 222 kinjup60n_kzzslope0pt6.pun 168 kinjup60n_kzzslope0pt7.pun 119 kinjup60n_kzzslope0pt8.pun 74 kinjup60n_kzzslope0pt9.pun 35 kinjup60n_kzzslope1pt0.pun 4.5 kinjup60n_kzzslope1pt1.pun 0.52 kinjup60n_kzzslope1pt2.pun 0.52