On the Spatial Distribution of Minor Species in Jupiter’s Troposphere as Inferred From Juno JIRAM Data
dc.contributor.author | Grassi, D. | |
dc.contributor.author | Adriani, A. | |
dc.contributor.author | Mura, A. | |
dc.contributor.author | Atreya, S. K. | |
dc.contributor.author | Fletcher, L. N. | |
dc.contributor.author | Lunine, J. I. | |
dc.contributor.author | Orton, G. S. | |
dc.contributor.author | Bolton, S. | |
dc.contributor.author | Plainaki, C. | |
dc.contributor.author | Sindoni, G. | |
dc.contributor.author | Altieri, F. | |
dc.contributor.author | Cicchetti, A. | |
dc.contributor.author | Dinelli, B. M. | |
dc.contributor.author | Filacchione, G. | |
dc.contributor.author | Migliorini, A. | |
dc.contributor.author | Moriconi, M. L. | |
dc.contributor.author | Noschese, R. | |
dc.contributor.author | Olivieri, A. | |
dc.contributor.author | Piccioni, G. | |
dc.contributor.author | Sordini, R. | |
dc.contributor.author | Stefani, S. | |
dc.contributor.author | Tosi, F. | |
dc.contributor.author | Turrini, D. | |
dc.date.accessioned | 2020-04-02T18:39:05Z | |
dc.date.available | WITHHELD_13_MONTHS | |
dc.date.available | 2020-04-02T18:39:05Z | |
dc.date.issued | 2020-04 | |
dc.identifier.citation | Grassi, D.; Adriani, A.; Mura, A.; Atreya, S. K.; Fletcher, L. N.; Lunine, J. I.; Orton, G. S.; Bolton, S.; Plainaki, C.; Sindoni, G.; Altieri, F.; Cicchetti, A.; Dinelli, B. M.; Filacchione, G.; Migliorini, A.; Moriconi, M. L.; Noschese, R.; Olivieri, A.; Piccioni, G.; Sordini, R.; Stefani, S.; Tosi, F.; Turrini, D. (2020). "On the Spatial Distribution of Minor Species in Jupiter’s Troposphere as Inferred From Juno JIRAM Data." Journal of Geophysical Research: Planets 125(4): n/a-n/a. | |
dc.identifier.issn | 2169-9097 | |
dc.identifier.issn | 2169-9100 | |
dc.identifier.uri | https://hdl.handle.net/2027.42/154637 | |
dc.description.abstract | The spatial distribution of water, ammonia, phosphine, germane, and arsine in the Jupiter’s troposphere has been inferred from the Jovian Infrared Auroral Mapper (JIRAM) Juno data. Measurements allow us to retrieve the vertically averaged concentration of gases between ~3 and 5 bars from infrared‐bright spectra. Results were used to create latitudinal profiles. The water vapor relative humidity varies with latitude from <1% to over 15%. At intermediate latitudes (30–70°) the water vapor maxima are associated with the location of cyclonic belts, as inferred from mean zonal wind profiles (Porco et al., 2003). The high‐latitude regions (beyond 60°) are drier in the north (mean relative humidity around 2–3%) than the south, where humidity reaches 15% around the pole. The ammonia volume mixing ratio varies from 1 × 10−4 to 4 × 10−4. A marked minimum exists around 10°N, while data suggest an increase over the equator. The high‐latitude regions are different in the two hemispheres, with a gradual increase in the south and more constant values with latitude in the north. The phosphine volume mixing ratio varies from 4 × 10−7 to 10 × 10−7. A marked minimum exists in the North Equatorial Belt. For latitudes poleward 30°S and 30°N, the northern hemisphere appears richer in phosphine, with a decrease toward the pole, while the opposite is observed in the south. JIRAM data indicate an increase of germane volume mixing ratio from 2 × 10−10 to 8 × 10−10 from both poles to 15°S, with a depletion centered around the equator. Arsine presents the opposite trend, with maximum values of 6 × 10−10 at the two poles and minima below 1 × 10−10 around 20°S.Key PointsHorizontal variations of gases are dominated by latitudinal components; longitudinal variations are relatively more important for waterPhosphine and germane abundances fit well the model of disequilibrium species transported upward from deep troposphere by vertical mixingStrong upturn of arsine at polar latitudes seen by JIRAM cannot be explained by the diffusion‐kinetics model | |
dc.publisher | Springer | |
dc.publisher | Wiley Periodicals, Inc. | |
dc.subject.other | Jupiter | |
dc.subject.other | atmospheric composition | |
dc.subject.other | minor gases | |
dc.title | On the Spatial Distribution of Minor Species in Jupiter’s Troposphere as Inferred From Juno JIRAM Data | |
dc.type | Article | |
dc.rights.robots | IndexNoFollow | |
dc.subject.hlbsecondlevel | Geological Sciences | |
dc.subject.hlbtoplevel | Science | |
dc.description.peerreviewed | Peer Reviewed | |
dc.description.bitstreamurl | https://deepblue.lib.umich.edu/bitstream/2027.42/154637/1/jgre21310_am.pdf | |
dc.description.bitstreamurl | https://deepblue.lib.umich.edu/bitstream/2027.42/154637/2/jgre21310.pdf | |
dc.description.bitstreamurl | https://deepblue.lib.umich.edu/bitstream/2027.42/154637/3/jgre21310-sup-0001-2019JE006206-SI.pdf | |
dc.identifier.doi | 10.1029/2019JE006206 | |
dc.identifier.source | Journal of Geophysical Research: Planets | |
dc.identifier.citedreference | Orton, G. S., Momary, T., Ingersoll, A. P., Adriani, A., Hansen, C. J., Janssen, M., Arballo, J., Atreya, S. K., Bolton, S., Brown, S., Caplinger, M., Grassi, D., Li, C., Levin, S., Moriconi, M. L., Mura, A., & Sindoni, G. ( 2017 ). Multiple‐wavelength sensing of Jupiter during the Juno mission’s first perijove passage. Geophysical Research Letters, 44, 4607 – 4614. https://doi.org/10.1002/2017GL073019 | |
dc.identifier.citedreference | Fletcher, L. N., Orton, G. S., Rogers, J. H., Giles, R. S., Payne, A. V., Irwin, P. G. J., & Vedovato, M. ( 2017 ). Moist convection and the 2010–2011 revival of Jupiter’s South Equatorial Belt. Icarus, 286, 94 – 117. https://doi.org/10.1016/j.icarus.2017.01.001 | |
dc.identifier.citedreference | Fletcher, L. N., Orton, G. S., Teanby, N. A., & Irwin, P. G. J. ( 2009 ). Phosphine on Jupiter and Saturn from Cassini/CIRS. Icarus, 202 ( 2 ), 543 – 564. https://doi.org/10.1016/j.icarus.2009.03.023 | |
dc.identifier.citedreference | Gierasch, P. J., Conrath, B. J., & Magalha˜es, J. A. ( 1986 ). Zonal mean properties of Jupiter’s upper troposphere from Voyager infrared observations. Icarus, 67 ( 3 ), 456 – 483. https://doi.org/10.1016/0019‐1035(86)90125‐9 | |
dc.identifier.citedreference | Giles, R. S., Fletcher, L. N., & Irwin, P. G. J. ( 2015 ). Cloud structure and composition of Jupiter’s troposphere from 5‐μm Cassini VIMS spectroscopy. Icarus, 257, 457 – 470. https://doi.org/10.1016/j.icarus.2015.05.030 | |
dc.identifier.citedreference | Giles, R. S., Fletcher, L. N., & Irwin, P. G. J. ( 2017 ). Latitudinal variability in Jupiter’s tropospheric disequilibrium species: GeH 4, AsH 3 and PH 3. Icarus, 289, 254 – 269. https://doi.org/10.1016/j.icarus.2016.10.023 | |
dc.identifier.citedreference | Giles, R. S., Fletcher, L. N., Irwin, P. G. J., Orton, G. S., & Sinclair, J. A. ( 2017 ). Ammonia in Jupiter’s troposphere from high‐resolution 5 μm spectroscopy. Geophysical Research Letters, 44, 10,838 – 10,844. https://doi.org/10.1002/2017GL075221 | |
dc.identifier.citedreference | Gordon, I. E., Rothman, L. S., Hill, C., Kochanov, R. V., Tan, Y., Bernath, P. F., Birk, M., Boudon, V., Campargue, A., Chance, K. V., Drouin, B. J., Flaud, J. M., Gamache, R. R., Hodges, J. T., Jacquemart, D., Perevalov, V. I., Perrin, A., Shine, K. P., Smith, M. A. H., Tennyson, J., Toon, G. C., Tran, H., Tyuterev, V. G., Barbe, A., Császár, A. G., Devi, V. M., Furtenbacher, T., Harrison, J. J., Hartmann, J. M., Jolly, A., Johnson, T. J., Karman, T., Kleiner, I., Kyuberis, A. A., Loos, J., Lyulin, O. M., Massie, S. T., Mikhailenko, S. N., Moazzen‐Ahmadi, N., Müller, H. S. P., Naumenko, O. V., Nikitin, A. V., Polyansky, O. L., Rey, M., Rotger, M., Sharpe, S. W., Sung, K., Starikova, E., Tashkun, S. A., Auwera, J. V., Wagner, G., Wilzewski, J., Wcisło, P., Yu, S., & Zak, E. J. ( 2017 ). The HITRAN2016 molecular spectroscopic database. Journal of Quantitative Spectroscopy and Radiative Transfer, 203, 3 – 69. https://doi.org/10.1016/j.jqsrt.2017.06.038 | |
dc.identifier.citedreference | Grassi, D., Adriani, A., Moriconi, M. L., Ignatiev, N. I., D’Aversa, E., Colosimo, F., Negrão, A., Brower, L., Dinelli, B. M., Coradini, A., & Piccioni, G. ( 2010 ). Jupiter’s hot spots: Quantitative assessment of the retrieval capabilities of future IR spectro‐imagers. Planetary and Space Science, 58 ( 10 ), 1265 – 1278. https://doi.org/10.1016/j.pss.2010.05.003 | |
dc.identifier.citedreference | Grassi, D., Adriani, A., Mura, A., Dinelli, B. M., Sindoni, G., Turrini, D., Filacchione, G., Migliorini, A., Moriconi, M. L., Tosi, F., Noschese, R., Cicchetti, A., Altieri, F., Fabiano, F., Piccioni, G., Stefani, S., Atreya, S., Lunine, J., Orton, G., Ingersoll, A., Bolton, S., Levin, S., Connerney, J., Olivieri, A., & Amoroso, M. ( 2017 ). Preliminary results on the composition of Jupiter’s troposphere in hot spot regions from the JIRAM/Juno instrument. Geophysical Research Letters, 44, 4615 – 4624. https://doi.org/10.1002/2017GL072841 | |
dc.identifier.citedreference | Grassi, D., Ignatiev, N. I., Sindoni, G., d’Aversa, E., Maestri, T., Adriani, A., Mura, A., Filacchione, G., Dinelli, B. M., Noschese, R., Cicchetti, A., Piccioni, G., Turrini, D., Tosi, F., Moriconi, M. L., Olivieri, A., Plainaki, C., Amoroso, M., Atreya, S. K., Orton, G. S., & Bolton, S. ( 2017 ). Analysis of IR‐bright regions of Jupiter in JIRAM‐Juno data: Methods and validation of algorithms. Journal of Quantitative Spectroscopy and Radiative Transfer, 202, 200 – 209. https://doi.org/10.1016/j.jqsrt.2017.08.008 | |
dc.identifier.citedreference | Ingersoll, A. P., Dowling, T. E., Gierasch, P. J., Orton, G. S., Read, P. L., Sánchez‐Lavega, A., Showman, A. P., Simon‐Miller, A. A., & Vasavada, A. R. ( 2004 ). Dynamic of Jupiter’s atmosphere, in Jupiter, the planet, satellite and magnetosphere, Bagenal, Dowling and McKinnon ed. Cambridge: Cambridge University Press. ISBN: 0521818087. | |
dc.identifier.citedreference | Irwin, P. G., Weir, A. L., Taylor, F. W., Calcutt, S. B., & Carlson, R. W. ( 2001 ). The origin of belt/zone contrasts in the atmosphere of Jupiter and their correlation with 5‐μm opacity. Icarus, 149 ( 2 ), 397 – 415. https://doi.org/10.1006/icar.2000.6542 | |
dc.identifier.citedreference | Irwin, P. G. J., Teanby, N. A., de Kok, R., Fletcher, L. N., Howett, C. J. A., Tsang, C. C. C., Wilson, C. F., Calcutt, S. B., Nixon, C. A., & Parrish, P. D. ( 2007 ). The NEMESIS planetary atmosphere radiative transfer and retrieval tool. Journal of Quantitative Spectroscopy and Radiative Transfer, 109, 1136 – 1150. https://doi.org/10.1016/j.jqsrt.2007.11.006 | |
dc.identifier.citedreference | Irwin, P. G. J., Weir, A. L., Smith, S. E., Taylor, F. W., Lambert, A. L., Calcutt, S. B., Cameron‐Smith, P. J., Carlson, R. W., Baines, K., Orton, G. S., Drossart, P., Encrenaz, T., & Roos‐Serote, M. ( 1998 ). Cloud structure and atmospheric composition of Jupiter retrieved from Galileo near‐infrared mapping spectrometer real‐time spectra. Journal of Geophysical Research, 103 ( E10 ), 23001 – 23021. https://doi.org/10.1029/98JE00948 | |
dc.identifier.citedreference | Jacquinet‐Husson, N., Arié, E., Ballard, J., Barbe, A., Bjoraker, G., Bonnet, B., Brown, L. R., Camy‐Peyret, C., Champion, J. P., Chédin, A., Chursin, A., Clerbaux, C., Duxbury, G., Flaud, J. M., Fourrié, N., Fayt, A., Graner, G., Gamache, R., Goldman, A., Golovko, V., Guelachvili, G., Hartmann, J. M., Hilico, J. C., Hillman, J., Lefèvre, G., Lellouch, E., Mikhaı̈lenko, S. N., Naumenko, O. V., Nemtchinov, V., Newnham, D. A., Nikitin, A., Orphal, J., Perrin, A., Reuter, D. C., Rinsland, C. P., Rosenmann, L., Rothman, L. S., Scott, N. A., Selby, J., Sinitsa, L. N., Sirota, J. M., Smith, A. M., Smith, K. M., Tyuterev, V. G., Tipping, R. H., Urban, S., Varanasi, P., & Weber, M. ( 1999 ). The 1997 spectroscopic GEISA databank. Journal of Quantitative Spectroscopy and Radiative Transfer, 62 ( 2 ), 205 – 254. https://doi.org/10.1016/S0022‐4073(98)00111‐3 | |
dc.identifier.citedreference | Kylling, A., Stamnes, K., & Tsay, S.. C. ( 1995 ). A reliable and efficient two‐stream algorithm for spherical radiative transfer: Documentation of accuracy in realistic layered media. Journal of Atmospheric Chemistry, 21 ( 2 ), 115 – 150. https://doi.org/10.1007/BF00696577 | |
dc.identifier.citedreference | Li, C., Ingersoll, A., Janssen, M., Levin, S., Bolton, S., Adumitroaie, V., Allison, M., Arballo, J., Bellotti, A., Brown, S., Ewald, S., Jewell, L., Misra, S., Orton, G., Oyafuso, F., Steffes, P., & Williamson, R. ( 2017 ). The distribution of ammonia on Jupiter from a preliminary inversion of Juno microwave radiometer data. Geophysical Research Letters, 44, 5317 – 5325. https://doi.org/10.1002/2017GL073159 | |
dc.identifier.citedreference | McInnes, L., Healy, J., & Astels, S. ( 2017 ). Hdbscan: Hierarchical density based clustering. Journal of Open Source Software, 2 ( 11 ), 205. https://doi.org/10.21105/joss.00205 | |
dc.identifier.citedreference | Noschese, R., and Adriani, A., ( 2017 ), JNO‐J‐JIRAM‐3‐RDR‐V1.0, NASA Planetary Data System, https://pds‐atmospheres.nmsu.edu/data_and_services/atmospheres_data/JUNO/jiram.html | |
dc.identifier.citedreference | Porco, C., West, R. A., McEwen, A., del Genio, A., Ingersoll, A. P., Thomas, P., Squyres, S., Dones, L., Murray, C. D., Johnson, T. V., Burns, J. A., Brahic, A., Neukum, G., Veverka, J., Barbara, J. M., Denk, T., Evans, M., Ferrier, J. J., Geissler, P., Helfenstein, P., Roatsch, T., Throop, H., Tiscareno, M., & Vasavada, A. R. ( 2003 ). Cassini imaging of Jupiter’s atmosphere, satellites, and rings. Science, 299 ( 5612 ), 1541 – 1547. https://doi.org/10.1126/science.1079462 | |
dc.identifier.citedreference | Prinn, R. G., & Barshay, S. S. ( 1977 ). Carbon monoxide on Jupiter and implications for atmospheric convection. Science, 198 ( 4321 ), 1031 – 1034. https://doi.org/10.1126/science.198.4321.1031‐a | |
dc.identifier.citedreference | Robinson, T. D., & Catling, D. C. ( 2013 ). Common 0.1 bar tropopause in thick atmospheres set by pressure‐dependent infrared transparency. Nature Geoscience, 7. https://doi.org/10.1038/ngeo2020 | |
dc.identifier.citedreference | Rodgers, C. R. ( 2000 ). Inverse methods for atmospheric sounding: Theory and practice. Singapore: World Scientific. ISBN: 9789810227401. | |
dc.identifier.citedreference | Rogers, J. H. ( 2009 ). The giant planet Jupiter. Cambridge University Press, ISBN‐13, 978 – 0521115308. | |
dc.identifier.citedreference | Roos‐Serote, M., Drossart, P., Encrenaz, T., Lellouch, E., Carlson, R. W., Baines, K. H., Kamp, L., Mehlman, R., Orton, G. S., Calcutt, S., Irwin, P., Taylor, F., & Weir, A. ( 1998 ). Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia. Journal of Geophysical Research, 103 ( E10 ). https://doi.org/10.1029/98JE01049 | |
dc.identifier.citedreference | Roos‐Serote, M., Vasavada, A. R., Kamp, L., Drossart, P., Irwin, P., Nixon, C., & Carlson, R. W. ( 2000 ). Proximate humid and dry regions in Jupiter’s atmosphere indicate complex local meteorology. Nature, 405 ( 6783 ), 158 – 160. https://doi.org/10.1038/35012023 | |
dc.identifier.citedreference | Schaeffer, R. D., & Lovejoy, R. W. ( 1985 ). Absolute line strengths of 74 GeH 4 near 5 μm. Journal of Molecular Spectroscopy, 113. https://doi.org/10.1016/0022‐2852(85)90270‐X | |
dc.identifier.citedreference | Seiff, A., Kirk, D. B., Knight, T. C. D., Young, R. E., Mihalov, J. D., Young, L. A., Milos, F. S., Schubert, G., Blanchard, R. C., & Atkinson, D. ( 1998 ). Thermal structure of Jupiter’s atmosphere near the edge of a 5‐μm hot spot in the north equatorial belt. Journal of Geophysical Research, 103 ( E10 ), 22857 – 22889. https://doi.org/10.1029/98JE01766. Available as numerical data as GP‐J‐ASI‐3‐ENTRY‐V1.0, NASA Planetary Data System | |
dc.identifier.citedreference | Showman, A. P., & Ingersoll, A. P. ( 1998 ). Interpretation of Galileo probe data and implications for Jupiter’s dry downdrafts. Icarus, 132. https://doi.org/10.1006/icar.1998.5898 | |
dc.identifier.citedreference | Siegel, S. ( 1956 ). Non‐parametric statistics for the behavioral sciences. New York: McGraw‐Hill. ISBN: 0070856893. | |
dc.identifier.citedreference | Sindoni, G., Grassi, D., Adriani, A., Mura, A., Moriconi, M. L., Dinelli, B. M., Filacchione, G., Tosi, F., Piccioni, G., Migliorini, A., Altieri, F., Fabiano, F., Turrini, D., Noschese, R., Cicchetti, A., Stefani, S., Bolton, S. J., Connerney, J. E. P., Atreya, S. K., Bagenal, F., Hansen, C., Ingersoll, A., Janssen, M., Levin, S. M., Lunine, J. I., Orton, G., Olivieri, A., & Amoroso, M. ( 2017 ). Characterization of the white ovals on Jupiter’s Southern Hemisphere using the first data by the Juno/JIRAM instrument. Geophysical Research Letters, 44, 4660 – 4668. https://doi.org/10.1002/2017GL072940 | |
dc.identifier.citedreference | Taylor, F. W., Atreya, S. K., Encrenaz, Th., Hunten, D. M., Irwin, P. G. J., & Owen, T. C. ( 2004 ). The composition of the atmosphere of Jupiter, in Jupiter, the planet, satellite and magnetosphere, Bagenal, Dowling and McKinnon ed. Cambridge: Cambridge University Press. ISBN: 0521818087. | |
dc.identifier.citedreference | Tollefson, J., Wong, M. H., de Pater, I., Simon, A. A., Orton, G. S., Rogers, J. H., Atreya, S. K., Cosentino, R. G., Januszewski, W., Morales‐Juberías, R., & Marcus, P. S. ( 2017 ). Changes in Jupiter’s zonal wind profiles preceding and during the Juno mission. Icarus, 296, 163 – 178. https://doi.org/10.1016/j.icarus.2017.06.007 | |
dc.identifier.citedreference | Visscher, C., & Fegley, B. ( 2005 ). Chemical constraints on the water and total oxygen abundances in the deep atmosphere of Saturn. The Astrophysical Journal, 623. https://doi.org/10.1086/428493 | |
dc.identifier.citedreference | Visscher, C., & Moses, J. I. ( 2011 ). Quenching of carbon monoxide and methane in the atmospheres of cool brown dwarfs and hot Jupiters. The Astrophysical Journal, 783 ( 1 ). https://doi.org/10.1088/0004‐637X/738/1/72 | |
dc.identifier.citedreference | Wallace, J., & Hobbs, P. ( 2006 ). Atmospheric science. An introductory survey. London: Academic Press. ISBN: 9780127329512. | |
dc.identifier.citedreference | Wang, D., Gierasch, P. J., Lunine, J. I., & Mousis, O. ( 2015 ). New insights on Jupiter’s deep water abundance from disequilibrium species. Icarus, 250, 154 – 164. https://doi.org/10.1016/j.icarus.2014.11.026 | |
dc.identifier.citedreference | Wang, D., Lunine, J. I., & Mousis, O. ( 2016 ). Modeling the disequilibrium species for Jupiter and Saturn: Implications for Juno and Saturn entry probe. Icarus, 276, 21 – 38. https://doi.org/10.1016/j.icarus.2016.04.027 | |
dc.identifier.citedreference | Wenger, C., & Champion, J. P. ( 1998 ). Spherical top data system (STDS) software for the simulation of spherical top spectra. Journal of Quantitative Spectroscopy and Radiative Transfer, 59. https://doi.org/10.1016/S0022‐4073(97)00106‐4 | |
dc.identifier.citedreference | Young, R. M. B., Read, P. L., & Wang, Y. ( 2018 ). Simulating Jupiter’s weather layer. Part I: Jet spin‐up in a dry atmosphere. Icarus, 326, 225 – 252. https://doi.org/10.1016/j.icarus.2018.12.005 | |
dc.identifier.citedreference | Achterberg, R. K., Conrath, B. J., & Gierasch, P. J. ( 2006 ). Cassini CIRS retrievals of ammonia in Jupiter’s upper troposphere. Icarus, 182. https://doi.org/10.1016/j.icarus.2005.12.020 | |
dc.identifier.citedreference | Stamnes, K., Tsay, S. C., Wiscombe, W., & Jayaweera, K. ( 1998 ). Numerically stable algorithm for discrete‐ordinate‐method radiative transfer in multiple scattering and emitting layered media. Applied Optics, 27 ( 12 ), 2502 – 2509. https://doi.org/10.1364/AO.27.002502 | |
dc.identifier.citedreference | Adriani, A., Filacchione, G., Iorio, T., Turrini, D., Noschese, R., Cicchetti, A., Grassi, D., Mura, A., Sindoni, G., Zambelli, M., Piccioni, G., Capria, M. T., Tosi, F., Orosei, R., Dinelli, B. M., Moriconi, M. L., Roncon, E., Lunine, J. I., Becker, H. N., Bini, A., Barbis, A., Calamai, L., Pasqui, C., Nencioni, S., Rossi, M., Lastri, M., Formaro, R., & Olivieri, A. ( 2014 ). JIRAM, the Jovian Infrared Auroral Mapper. Space Science Reviews, 213 ( 1‐4 ), 393 – 446. https://doi.org/10.1007/s11214‐014‐0094‐y | |
dc.identifier.citedreference | Adriani, A., Moriconi, M. L., Mura, A., Tosi, F., Sindoni, G., Noschese, R., Cicchetti, A., & Filacchione, G. ( 2016 ). Juno’s Earth flyby: The Jovian Infrared Auroral Mapper preliminary results. Astrophysics and Space Science, 361 ( 8 ), 1 – 8. https://doi.org/10.1007/s10509‐016‐2842‐9 | |
dc.identifier.citedreference | Adriani, A., Bracco, A., Grassi, D., Moriconi, M. L., Mura, A., Orton, G. S., Altieri, F., Ingersoll, A., Atreya, S. K., Lunine, J. I., Migliorini, A., Noschese, R., Cicchetti, A., Sordini, R., Sindoni, G., Plainaki, C., Dinelli, B. M., Turrini, D., Filacchione, G., Piccioni, G., Tosi, F., & Bolton, S. ( 2020 ). Two‐years observations of the Jupiter polar regions by JIRAM on board Juno, in press on. Journal of Geophysical Research Planets. https://doi.org/10.1029/2019JE006098 | |
dc.identifier.citedreference | Antuñano, A., Fletcher, L. N., Orton, G. S., Melin, H., Rogers, J. H., Harrington, J., Donnelly, P. T., Rowe‐Gurney, N., & Blake, J. S. D. ( 2018 ). Infrared characterization of Jupiter’s equatorial disturbance cycle. Geophysical Research Letters, 45 ( 20 ). https://doi.org/10.1029/2018GL080382 | |
dc.identifier.citedreference | Archinal, B. A., A’Hearn, M. F., Bowell, E., Conrad, A., Consolmagno, G. J., Courtin, R., Fukushima, T., Hestroffer, D., Hilton, J. L., Krasinsky, G. A., Neumann, G., Oberst, J., Seidelmann, P. K., Stooke, P., Tholen, D. J., Thomas, P. C., & Williams, I. P. ( 2011 ). Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2009. Celestial Mechanics and Dynamical Astronomy, 109 ( 2 ), 101 – 135. https://doi.org/10.1007/s10569‐010‐9320‐4 | |
dc.identifier.citedreference | Atreya, S. K., Wong, M. H., Owen, T. C., Mahaffy, P. R., Niemann, H. B., de Pater, I., Drossart, P., & Encrenaz, T. ( 1999 ). A comparison of the atmospheres of Jupiter and Saturn: Deep atmospheric composition, cloud structure, vertical mixing, and origin. Planetary and Space Science, 47 ( 10–11 ), 1243 – 1262. https://doi.org/10.1016/S0032‐0633(99)00047‐1 | |
dc.identifier.citedreference | Bjoraker, G. L., Wong, M. H., Pater, I.., & Ádámkovics, M. ( 2015 ). Jupiter’s deep cloud structure revealed using Keck observations of spectrally resolved line shape. The Astrophysical Journal, 810 ( 2 ), 122. https://doi.org/10.1088/0004‐637x/810/2/122 | |
dc.identifier.citedreference | Blain, D., Fouchet, T., Greathouse, T., Encrenaz, T., Charnay, B., Bézard, B., Li, C., Lellouch, E., Orton, G., N. Fletcher, L., & Drossart, P. ( 2018 ). Mapping of Jupiter’s tropospheric NH 3 abundance using ground‐based IRTF/TEXES observations at 5 μm. Icarus, 314, 106 – 120. https://doi.org/10.1016/j.icarus.2018.06.002 | |
dc.identifier.citedreference | Bolton, S., Adriani, A., Adumitroaie, V., Allison, M., Anderson, J., Atreya, S., Bloxham, J., Brown, S., Connerney, J. E. P., DeJong, E., Folkner, W., Gautier, D., Grassi, D., Gulkis, S., Guillot, T., Hansen, C., Hubbard, W. B., Iess, L., Ingersoll, A., Janssen, M., Jorgensen, J., Kaspi, Y., Levin, S. M., Li, C., Lunine, J., Miguel, Y., Mura, A., Orton, G., Owen, T., Ravine, M., Smith, E., Steffes, P., Stone, E., Stevenson, D., Thorne, R., Waite, J., Durante, D., Ebert, R. W., Greathouse, T. K., Hue, V., Parisi, M., Szalay, J. R., & Wilson, R. ( 2017 ). Jupiter’s interior and deep atmosphere: The initial pole‐to‐pole passes with the Juno spacecraft. Science, 356 ( 6340 ), 821 – 825. https://doi.org/10.1126/science.aal2108 | |
dc.identifier.citedreference | Boudon, V., Grigoryan, T., Philipot, F., Richard, C., Tchana, F. K., Manceron, L., Rizopoulos, A., Auwera, J. V., & Encrenaz, T. ( 2018 ). Line positions and intensities for the ν 3 band of 5 isotopologues of germane for planetary applications. Journal of Quantitative Spectroscopy and Radiative Transfer, 205, 174 – 183. https://doi.org/10.1016/j.jqsrt.2017.10.017 | |
dc.identifier.citedreference | Campello, R. J., Moulavi, D., & Sander, J. ( 2013 ). Density‐based clustering based on hierarchical density estimates. In Pacific‐ Asia conference on knowledge discovery and data mining (pp. 160 – 172 ). Berlin, Heidelberg: Springer. https://doi.org/10.1007/978‐3‐642‐37456‐2_14 | |
dc.identifier.citedreference | Conrath, B. J., Gierasch, P. J., & Ustinov, E. A. ( 1998 ). Thermal structure and para hydrogen fraction on the outer planets from Voyager IRIS measurements. Icarus, 135 ( 2 ), 501 – 517. https://doi.org/10.1006/icar.1998.6000 | |
dc.identifier.citedreference | de Pater, I., Sault, R. J., Butler, B., DeBoer, D., & Wong, M. H. ( 2016 ). Peering through Jupiter’s clouds with radio spectral imaging. Science, 352 ( 6290 ), 1198 – 1201. https://doi.org/10.1126/science.aaf2210 | |
dc.identifier.citedreference | Dowling, T. E., & Gierasch, P. J. ( 1989 ). Cyclones and moist convection on Jovian planets. Bulletin of the American Astronomical Society, 21. | |
dc.identifier.citedreference | Drossart, P., Lellouch, E., Bézard, B., Maillard, J. P., & Tarrago, G. ( 1990 ). Jupiter: Evidence for a phosphine enhancement at high northern latitudes. Icarus, 83 ( 1 ), 248 – 253. https://doi.org/10.1016/0019‐1035(90)90018‐5 | |
dc.identifier.citedreference | Drossart, P., Roos‐Serote, M., Encrenaz, T., Lellouch, E., Baines, K. H., Carlson, R. W., Kamp, L. W., Orton, G. S., Calcutt, S., Irwin, P., Taylor, F. W., & Weir, A. ( 1998 ). The solar reflected component in Jupiter’s 5‐μm spectra from NIMS/Galileo observations. Journal of Geophysical Research, 103 ( E10 ), 23043 – 23049. https://doi.org/10.1029/98JE01899 | |
dc.identifier.citedreference | Fegley, B., & Prinn, R. G. ( 1985 ). Equilibrium and nonequilibrium chemistry of Saturn’s atmosphere—Implications for the observability of PH 3, N 2, CO, and GeH 4. The Astrophysical Journal, 299. https://doi.org/10.1086/163775 | |
dc.identifier.citedreference | Fletcher L., Antunano A., Orton G., Greathouse T., Melin H., Donnelly P., Rogers J., & Mettig H. J. ( 2019 ) Jupiter’s ammonia‐rich equatorial plumes, contribution 453‐1 to the EPSC‐DPS Joint Meeting 2019, https://meetingorganizer.copernicus.org/EPSC‐DPS2019/EPSC‐DPS2019‐453‐1.pdf | |
dc.identifier.citedreference | Fletcher, L. N. ( 2017 ). Cycles of activity in the Jovian atmosphere. Geophysical Research Letters, 44, 4725 – 4729. https://doi.org/10.1002/2017GL073806 | |
dc.identifier.citedreference | Fletcher, L. N., Greathouse, T. K., Orton, G. S., Sinclair, J. A., Giles, R. S., Irwin, P. G. J., & Encrenaz, T. ( 2016 ). Mid‐infrared mapping of Jupiter’s temperatures, aerosol opacity and chemical distributions with IRTF/TEXES. Icarus, 278, 128 – 161. https://doi.org/10.1016/j.icarus.2016.06.008 | |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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