First Observations of CH4 and H3+ ${mathrm{H}}_{3}^{+}$ Spatially Resolved Emission Layers at Jupiter Equator, as Seen by JIRAM/Juno
dc.contributor.author | Migliorini, A. | |
dc.contributor.author | Dinelli, B. M. | |
dc.contributor.author | Castagnoli, C. | |
dc.contributor.author | Moriconi, M. L. | |
dc.contributor.author | Altieri, F. | |
dc.contributor.author | Atreya, S. | |
dc.contributor.author | Adriani, A. | |
dc.contributor.author | Mura, A. | |
dc.contributor.author | Tosi, F. | |
dc.contributor.author | Moirano, A. | |
dc.contributor.author | Piccioni, G. | |
dc.contributor.author | Grassi, D. | |
dc.contributor.author | Sordini, R. | |
dc.contributor.author | Noschese, R. | |
dc.contributor.author | Cicchetti, A. | |
dc.contributor.author | Bolton, S. J. | |
dc.contributor.author | Sindoni, G. | |
dc.contributor.author | Plainaki, C. | |
dc.contributor.author | Olivieri, A. | |
dc.date.accessioned | 2023-04-04T17:41:31Z | |
dc.date.available | 2024-04-04 13:41:29 | en |
dc.date.available | 2023-04-04T17:41:31Z | |
dc.date.issued | 2023-03 | |
dc.identifier.citation | Migliorini, A.; Dinelli, B. M.; Castagnoli, C.; Moriconi, M. L.; Altieri, F.; Atreya, S.; Adriani, A.; Mura, A.; Tosi, F.; Moirano, A.; Piccioni, G.; Grassi, D.; Sordini, R.; Noschese, R.; Cicchetti, A.; Bolton, S. J.; Sindoni, G.; Plainaki, C.; Olivieri, A. (2023). "First Observations of CH4 and H3+ ${mathrm{H}}_{3}^{+}$ Spatially Resolved Emission Layers at Jupiter Equator, as Seen by JIRAM/Juno." Journal of Geophysical Research: Planets 128(3): n/a-n/a. | |
dc.identifier.issn | 2169-9097 | |
dc.identifier.issn | 2169-9100 | |
dc.identifier.uri | https://hdl.handle.net/2027.42/176067 | |
dc.description.abstract | In this work, we present the detection of CH4 and H3+ ${mathrm{H}}_{3}^{+}$ emissions in the equatorial atmosphere of Jupiter as two well-separated layers located, respectively, at tangent altitudes of about 200 and 500–600 km above the 1-bar level using the observations of the Jovian InfraRed Auroral Mapper (JIRAM), on board Juno. This provides details of the vertical distribution of H3+ ${mathrm{H}}_{3}^{+}$ retrieving its Volume Mixing Ratio (VMR), concentration, and temperature. The thermal profile obtained from H3+ ${mathrm{H}}_{3}^{+}$ shows a peak of 600–800 K at about 550 km, with lower values than the ones reported in Seiff et al. (1998), https://doi.org/10.1029/98JE01766 above 500 km using VMR and temperature as free parameters and above 650 km when VMR is kept fixed with that model in the retrieval procedure. The observed deviations from the Galileo’s profile could potentially point to significant variability in the exospheric temperature with time. We suggest that vertically propagating waves are the most likely explanation for the observed VMR and temperature variations in the JIRAM data. Other possible phenomena could explain the observed evidence, for example, dynamic activity driving chemical species from lower layers toward the upper atmosphere, like the advection-diffusion processes, or precipitation by soft electrons, although better modeling is required to test these hypothesis. The characterization of CH4 and H3+ ${mathrm{H}}_{3}^{+}$ species, simultaneously observed by JIRAM, offers the opportunity for better constraining atmospheric models of Jupiter at equatorial latitudes.Plain Language SummaryThe Jovian Infrared Auroral Mapper (JIRAM) is the infrared imager and spectrometer on board the Juno mission, designed to investigate Jupiter’s atmosphere. A key objective of JIRAM is the investigation of the minor species, such as CH4 and H3+ ${mathrm{H}}_{3}^{+}$ that are very important to understanding the energy balance of the middle and upper atmosphere of Jupiter. These species have strong signatures in the 3.3–3.8 μm spectral region, well within the nominal wavelength range of the instrument. We present the analysis of recent images and spectra obtained by JIRAM, in the period December 2018–September 2020, plus additional measurements in March 2017, to study methane and H3+ ${mathrm{H}}_{3}^{+}$ vertical distribution at equatorial latitudes. We find that CH4 is localized around 200 km above the 1-bar level, while a distinct layer of H3+ ${mathrm{H}}_{3}^{+}$ is observed around 500–600 km (0.04–0.016 μbar). The observed vertical distribution and intensity variation of H3+ ${mathrm{H}}_{3}^{+}$ is likely to be the result of vertically propagating waves. However, other possible phenomena can be invoked to explain these findings, like for example, an uplifting of chemical species from lower layers toward the upper atmosphere, or soft electrons precipitation, although a rigorous modeling is needed to confirm the latter hypothesis.Key PointsDetection of CH4 and H3+ ${mathrm{H}}_{3}^{+}$ emissions over Jupiter’s disc as two well separated layers in the equatorial region at 200 and 600 kmThe H3+ ${mathrm{H}}_{3}^{+}$ temperature profile shows a peak of 600–800 K at about 600 km with some differences with respect to the Galileo’s profileThe observed features point out the presence of localized variability with altitude, perhaps indicative of wave activities | |
dc.publisher | Wiley Periodicals, Inc. | |
dc.publisher | Springer | |
dc.title | First Observations of CH4 and H3+ ${mathrm{H}}_{3}^{+}$ Spatially Resolved Emission Layers at Jupiter Equator, as Seen by JIRAM/Juno | |
dc.type | Article | |
dc.rights.robots | IndexNoFollow | |
dc.subject.hlbsecondlevel | Geological Sciences | |
dc.subject.hlbtoplevel | Science | |
dc.description.peerreviewed | Peer Reviewed | |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/176067/1/jgre22151.pdf | |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/176067/2/jgre22151_am.pdf | |
dc.identifier.doi | 10.1029/2022JE007509 | |
dc.identifier.source | Journal of Geophysical Research: Planets | |
dc.identifier.citedreference | Moore, L., Melin, H., O’Donoghue, J., Stallard, T. S., Moses, J. I., Galand, M., et al. ( 2019 ). Modelling H 3 + in planetary atmospheres: Effects of vertical gradients on observed quantities. Philosophical Transactions of the Royal Society A: Mathematical, Physical & Engineering Sciences, 377 ( 2154 ), 20190067. https://doi.org/10.1098/rsta.2019.0067 | |
dc.identifier.citedreference | Kim, S., Sim, C., Ho, J., Geballe, T. R., Yung, Y. L., Miller, S., & Kim, Y. H. ( 2015 ). Hot CH 4 in the polar regions of Jupiter. Icarus, 257, 217 – 220. https://doi.org/10.1016/j.icarus.2015.05.008 | |
dc.identifier.citedreference | Kim, S., Sim, C., Sohn, M., & Moses, J. ( 2014 ). CH 4 mixing ratios at microbar pressure levels of Jupiter a constrained by 3-micron ISO data. Icarus, 237, 42 – 51. https://doi.org/10.1016/j.icarus.2014.04.023 | |
dc.identifier.citedreference | Kita, H., Fujisawa, S., Tao, C., Kagitani, M., Sakanoi, T., & Kasaba, Y. ( 2018 ). Horizontal and vertical structures of Jovian infrared aurora: Observations using Subaru IRCS with adaptive optics. Icarus, 313, 93 – 106. https://doi.org/10.1016/j.icarus.2018.05.002 | |
dc.identifier.citedreference | Koskinen, T., Aylaward, A., & Miller, S. ( 2007 ). A stability limit for the atmospheres of giant extrasolar planets. Nature, 412 ( 7171 ), 891 – 848. https://doi.org/10.1038/nature06378 | |
dc.identifier.citedreference | Li, C., Ingersoll, A., Bolton, S., Levin, S., Janssen, M., Atreya, S., et al. ( 2020 ). The water abundance in Jupiter’s equatorial zone. Nature Astronomy, 4 ( 6 ), 609 – 616. https://doi.org/10.1038/s41550-020-1009-3 | |
dc.identifier.citedreference | Li, C., Ingersoll, A., Janssen, M., Levin, S., Bolton, S., Adumitroaie, V., et al. ( 2017 ). The distribution of ammonia on Jupiter from a preliminary inversion of Juno microwave radiometer data. Geophysical Research Letters, 44 ( 11 ), 5317 – 5325. https://doi.org/10.1002/2017GL073159 | |
dc.identifier.citedreference | Lindsay, C., & McCall, B. ( 2001 ). Comprehensive evaluation and compilation of H 3 + spectroscopy. Journal of Molecular Spectroscopy, 210 ( 1 ), 60 – 83. https://doi.org/10.1006/jmsp.2001.8444 | |
dc.identifier.citedreference | Lystrup, M., Miller, S., Dello Russo, N., Vervack, R., & Stallard, T. ( 2008 ). First vertical ion density profile in Jupiter’s auroral atmosphere: Direct observations using the Keck II telescope. The Astrophysical Journal, 677 ( 1 ), 790 – 797. https://doi.org/10.1086/529509 | |
dc.identifier.citedreference | Marten, A., De Bergh, C., Owen, T., Gautier, D., Maillard, J., Drossart, P., et al. ( 1994 ). Four micron high-resolution spectra of jupiter in the North equatorial belt: H 3 + emissions and the 12 C/ 13 C ratio. Planetary and Space Science, 42 ( 5 ), 391 – 399. https://doi.org/10.1016/0032-0633(94)90128-7 | |
dc.identifier.citedreference | Melin, H., Miller, S., Stallard, T., & Grodent, D. ( 2005 ). Non-LTE effects on H 3 + emission in the Jovian upper atmosphere. Icarus, 178 ( 1 ), 97 – 103. https://doi.org/10.1016/j.icarus.2005.04.016 | |
dc.identifier.citedreference | Melin, H., Stallard, T., O’Donoghue, J., Badman, S., Miller, S., & Blake, J. S. D. ( 2014 ). On the anticorrelation between H 3 + temperature and density in giant planet ionospheres. Monthly Notices of the Royal Astronomical Society, 438 ( 2 ), 1611 – 1617. https://doi.org/10.1093/mnras/stt2299 | |
dc.identifier.citedreference | Migliorini, A., Dinelli, B., Moriconi, M., Altieri, F., Adriani, A., Mura, A., et al. ( 2019 ). H 3 + characteristics in the Jupiter atmosphere as observed at limb with Juno/JIRAM. Icarus, 329, 132 – 139. https://doi.org/10.1016/j.icarus.2019.04.003 | |
dc.identifier.citedreference | Miller, S., Achilleos, N., Ballester, G. E., Lam, H. A., Tennyson, J., Geballe, T. R., & Trafton, L. M. ( 1997 ). Mid-to-low latitude H 3 + emission from Jupiter. Icarus, 130 ( 1 ), 57 – 67. https://doi.org/10.1006/icar.1997.5813 | |
dc.identifier.citedreference | Miller, S., Joseph, R. D., & Tennyson, J. ( 1990 ). Infrared emissions of H 3 + in the atmosphere of Jupiter in the 2.1 and 4.0 micron region. The Astrophysical Journal Letters, 360, L55. https://doi.org/10.1086/185811 | |
dc.identifier.citedreference | Miller, S., Tennyson, J., Geballe, T. R., & Stallard, T. ( 2020 ). Thirty years of H 3 + astronomy. Reviews of Modern Physics, 92 ( 3 ), 035003. https://doi.org/10.1103/RevModPhys.92.035003 | |
dc.identifier.citedreference | Moriconi, M., Adriani, A., Dinelli, B., Fabiano, F., Altieri, F., Tosi, F., et al. ( 2017 ). Preliminary JIRAM results from Juno polar observations: 3. Evidence of diffuse methane presence in the Jupiter auroral regions. Geophysical Research Letters, 44 ( 10 ), 4641 – 4648. https://doi.org/10.1002/2017GL073592 | |
dc.identifier.citedreference | Mura, A., Adriani, A., Connerney, J. E. P., Bolton, S., Altieri, F., Bagenal, F., et al. ( 2018 ). Juno observations of spot structures and a split tail in Io-induced aurorae on Jupiter. Science, 361 ( 6404 ), 774 – 777. https://doi.org/10.1126/science.aat1450 | |
dc.identifier.citedreference | Mura, A., Adriani, A., Altieri, F., Connerney, J. E. P., Bolton, S. J., Moriconi, M. L., et al. ( 2017 ). Infrared observations of Jovian aurora from Juno’s first orbit: Main oval and satellite footprints. Geophysical Research Letters, 44 ( 11 ), 5308 – 5316. https://doi.org/10.1022/2017GRL072954 | |
dc.identifier.citedreference | Noschese, R., & Adriani, A. ( 2017 ). Juno Jupiter JIRAM raw data archive v1.0. NASA Planetary Data System. https://doi.org/10.17189/FAY5-DE13 | |
dc.identifier.citedreference | O’Donoghue, J., Moore, L., Bhakyapaibul, T., Melin, H., Stallard, T., Connerney, J., & Tao, C. ( 2021 ). Global upper-atmospheric heating on Jupiter by the pola aurorae heating of Jupiter’s upper atmosphere above the great red spot. Nature, 596 ( 7870 ), 54 – 67. https://doi.org/10.1038/s41596-021-03706-w | |
dc.identifier.citedreference | O’Donoghue, J., Moore, L., Stallard, T., & Melin, H. ( 2016 ). Heating of Jupiter’s upper atmosphere above the great red spot. Nature, 536 ( 7615 ), 190 – 192. https://doi.org/10.1038/nature18940 | |
dc.identifier.citedreference | Ray, L., Lorch, C., O’Donoghue, J., Yates, J., Badman, S., Smith, C., & Stallard, T. ( 2019 ). Why is the H 3 + hot spot above Jupiter’s great red spot so hot? Philosophical Transaction of the Royal Society A, 377 ( 2154 ), 20180407. https://doi.org/10.1098/rsta.2018.0407 | |
dc.identifier.citedreference | Rodgers, C. D. ( 2000 ). Inverse methods for atmospheric sounding. World Scientific. https://doi.org/10.1142/3171 | |
dc.identifier.citedreference | Sada, P., Jennings, D., Romani, P., Bjoraker, G., Flasar, F., Kunde, V., et al. ( 2003 ). Transient IR phenomena observed by Cassini/CIRS in Jupiter’s auroral regions. Bulletin of the American Astronomical Society, 35, 402. | |
dc.identifier.citedreference | Sànchez-Lòpez, A., Lòpez-Puertas, M., Garcìa-Comas, M., Funke, B., Fouchet, T., & Snellen, I. ( 2022 ). The CH 4 abundance in Jupiter’s upper atmosphere. Astronomy and Astrophysics, 662, A91. https://doi.org/10.1051/0004-6361/202141933 | |
dc.identifier.citedreference | Satoh, T., & Connerney, J. ( 1999 ). Jupiter H 3 + emissions viewed in corrected Jovi magnetic coordinates. Icarus, 141 ( 2 ), 236 – 252. https://doi.org/10.1006/icar.1999.6173 | |
dc.identifier.citedreference | Seiff, A., Kirk, D. B., Knight, T. C. D., Young, R. E., Mihalov, J. D., Young, L. A., et al. ( 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 | |
dc.identifier.citedreference | Sinclair, J., Orton, G., Fernandes, J., Kasaba, Y., Sato, T. M., Fujiyoshi, T., et al. ( 2019 ). A brightening of Jupiter’s auroral 7.8-μm CH 4 emission during a solar-wind compression. Nature Astronomy, 3 ( 7 ), 607 – 613. https://doi.org/10.1038/s41550-019-0743-x | |
dc.identifier.citedreference | Sinclair, J. A., Orton, G., Greathouse, T., Fletcher, L., Tao, C., Gladstone, G. R., et al. ( 2017 ). Independent evolution of stratospheric temperatures in Jupiter’s northern and southern auroral regions from 2014 to 2016. Geophysical Research Letters, 44 ( 11 ), 5345 – 5354. https://doi.org/10.1002/2017GL073529 | |
dc.identifier.citedreference | Stallard, T., Burrell, A., Melin, H., Fletcher, L. N., Miller, S., Moore, L., et al. ( 2018 ). Identification of Jupiter’s magnetic equator within H 3 + ionospheric emission. Nature Astronomy, 2 ( 10 ), 773 – 777. https://doi.org/10.1038/s41550-018-0523-z | |
dc.identifier.citedreference | Stallard, T., Melin, H., Miller, S., Badman, S. V., Baines, K. H., Brown, R. H., et al. ( 2015 ). Cassini vims observations of H 3 + emission on the nightside of Jupiter. Journal of Geophysical Research: Space Physics, 120 ( 8 ), 6948 – 6973. https://doi.org/10.1002/2015JA021097 | |
dc.identifier.citedreference | Stallard, T., Melin, H., Miller, S., Moore, L., O’Donoghue, J., Connerney, J., et al. ( 2017 ). The great cold spot in Jupiter’s upper atmosphere. Geophysical Research Letters, 44 ( 7 ), 3000 – 3008. https://doi.org/10.1002/2016GL071956 | |
dc.identifier.citedreference | Tao, C., Badman, S., & Fujimoto, M. ( 2011 ). UV and IR auroral emission model for the outer planets: Jupiter and Saturn comparison. Icarus, 213 ( 2 ), 581 – 592. https://doi.org/10.1016/j.icarus.2011.04.001 | |
dc.identifier.citedreference | Uno, T., Yasaba, Y., Tao, C., Sakanoi, T., Kagitani, M., Fujisawa, S., et al. ( 2014 ). Vertical emissivity profiles of Jupiter’s northern H 3 + and h 2 infrared auroras observed by Subaru/IRCS. Journal of Geophysical Research: Space Physics, 119 ( 12 ), 10219 – 10241. https://doi.org/10.1002/2014JA020454 | |
dc.identifier.citedreference | Acton, C. H. ( 1996 ). Ancillary data services of NASA’s navigation and ancillary information facility. Planetary and Space Science, 44 ( 1 ), 65 – 70. https://doi.org/10.1016/0032-0633(95)00107-7 | |
dc.identifier.citedreference | Adriani, A., Filacchione, G., Di Iorio, T., Turrini, D., Noschese, R., Cicchetti, A., et al. ( 2017 ). 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., Mura, A., Moriconi, M., Dinelli, B. M., Fabiano, F., Altieri, F., et al. ( 2017 ). Preliminary JIRAM results from Juno polar observations: 2. Analysis of the Jupiter southern H 3 + emissions and comparison with the North aurora. Geophysical Research Letters, 44 ( 10 ), 4633 – 4640. https://doi.org/10.1002/2017GRL072905 | |
dc.identifier.citedreference | Altieri, F., Dinelli, B., Migliorini, A., Moriconi, M. L., Sindoni, G., Adriani, A., et al. ( 2016 ). Mapping of hydrocarbons and H 3 + emissions at Jupiter’s north pole using Galileo/NIMS data. Geophysical Research Letters, 43 ( 22 ), 11558 – 11566. https://doi.org/10.1002/2016GL070787 | |
dc.identifier.citedreference | Atreya, S. K. ( 1987 ). Atmospheres and ionospheres of the outer planets and their satellites (pp. 47 – 48 ). Springer. | |
dc.identifier.citedreference | Ballester, G. E., Miller, S., Tennyson, J., Trafton, L., & Geballe, T. ( 1994 ). Latitudinal temperature variations of Jovian H 3 +. Icarus, 107 ( 1 ), 189 – 194. https://doi.org/10.1006/icar.1994.1015 | |
dc.identifier.citedreference | Bonfond, B., Gladstone, G., Grodent, D., Greathause, T., Versteeg, M., Hue, V., et al. ( 2017 ). Morphology of the UV aurorae Jupiter during Juno’s first perijove observations. Geophysical Research Letters, 44 ( 10 ), 4463 – 4471. https://doi.org/10.1002/2017GL073114 | |
dc.identifier.citedreference | Bougher, S., Waite, J., Majeed, T., & Gladstone, G. ( 2005 ). Jupiter Thermospheric General Circulation Model (JTGCM): Global structure and dynamics driven by auroral and Joule heating. Journal of Geophysical Research, 110 ( E4 ), E04008. https://doi.org/10.1029/2003je002230 | |
dc.identifier.citedreference | Caldwell, J., Halthore, R., Orton, G., & Berstralh, J. ( 1988 ). Infrared polar brightenings on Jupiter VI. Spatial properties of methane emission. Icarus, 74 ( 2 ), 331 – 339. https://doi.org/10.1016/0019-1035(88)90045-0 | |
dc.identifier.citedreference | Caldwell, J., Tokunags, A., & Orton, G. ( 1983 ). Further observations of 8-μm polar brightenings of Jupiter. Icarus, 53 ( 1 ), 133 – 140. https://doi.org/10.1016/0019-1035(83)90026-x | |
dc.identifier.citedreference | Carlotti, M. ( 1988 ). Global-fit approach to the analysis of limb-scanning atmospheric measurements. Applied Optics, 27 ( 15 ), 3250 – 3254. https://doi.org/10.1364/ao.27.003250 | |
dc.identifier.citedreference | Clarke, J., Ajello, J., Ballester, G., Ben Jaffel, L., Connerney, J., Gerard, J. C., et al. ( 2002 ). Ultraviolet emissions from the magnetic footprints of Io, Ganymede, and Europa on Jupiter. Nature, 415 ( 6875 ), 997 – 1000. https://doi.org/10.1038/415997a | |
dc.identifier.citedreference | Connerney, J., Baron, R., Satoh, T., & Owen, T. ( 1993 ). Images of excited H 3 + at the foot of the Io flux tube in Jupiter’s atmosphere. Science, 262 ( 5136 ), 1035 – 1038. https://doi.org/10.1126/science.262.5136.1035 | |
dc.identifier.citedreference | Connerney, J., Timmins, S., Oliversen, R., Cao, H., Yadav, R. K., Stevenson, D. J., et al. ( 2022 ). A new model of Jupiter’s magnetic field at the completion of Juno’s prime mission. Journal of Geophysical Research: Planets, 127 ( 5 ), e2021JE007055. https://doi.org/10.1029/2021JE007138 | |
dc.identifier.citedreference | Cosentino, R., Morales-Juberias, R., Greathouse, T., Orton, G., Johnson, P., Fletcher, L., & Simon, A. ( 2017 ). New observations and modeling of Jupiter’s quasi-quadrennial oscillation. Journal of Geophysical Research: Planets, 122 ( 12 ), 2719 – 2744. https://doi.org/10.1002/2017JE005342 | |
dc.identifier.citedreference | Dinelli, B. ( 2021 ). Ch 4 and H 3 + retrieval results [Dataset]. Zenodo. https://doi.org/10.5281/zenodo.5658387 | |
dc.identifier.citedreference | Dinelli, B., Adriani, A., Mura, A., Altieri, F., Migliorini, A., & Moriconi, M. L. ( 2019 ). Juno/JIRAM’s view of Jupiter’s H 3 + emissions. Philosophical Transaction of the Royal Society A, 377 ( 2154 ), 20180406. https://doi.org/10.1098/rsta.2018.0406 | |
dc.identifier.citedreference | Drossart, P., Bezard, B., Atreya, S., Bishop, J., Waite, J. H., & Boice, D. ( 1993 ). Thermal profiles in the auroral regions of Jupiter. Journal of Geophysical Research, 98 ( E10 ), 18803 – 18812. https://doi.org/10.1029/93JE01801 | |
dc.identifier.citedreference | Drossart, P., Maillard, J.-P., Cladwell, S., Kim, S. J., Watson, J. K. G., Majewski, W. A., et al. ( 1989 ). Detection of the H 3 + on Jupiter. Nature, 340 ( 6234 ), 539 – 541. https://doi.org/10.1038/340539a0 | |
dc.identifier.citedreference | Gérard, J.-C., Mura, A., Bonfond, B., Gladstone, G., Adriani, A., Hue, V., et al. ( 2018 ). Concurrent ultraviolet and infrared observations of the north Jovian aurora during Juno’s first perijove. Icarus, 312, 145 – 156. https://doi.org/10.1016/j.icarus.2018.04.020 | |
dc.identifier.citedreference | Giles, R., Fletcher, L., Irwin, P., Melin, H., & Stallard, T. S. ( 2016 ). Detection of H 3 + auroral emission in the Jupiter’s 5-micron window. Astronomy and Astrophysics, 589, A67. https://doi.org/10.1051/0004-6361/201628170 | |
dc.identifier.citedreference | Grodent, D., Waite, J. J., & Gérard, J. ( 2001 ). A self-consistent model of the Jovian auroral thermal structure. Journal of Geophysical Research, 106 ( A7 ), 12933 – 12952. https://doi.org/10.1029/2000JA900129 | |
dc.identifier.citedreference | Hunten, D. M., & Dessler, A. J. ( 1977 ). Soft electrons as a possible heat source for Jupiter’s thermosphere. Planetary and Space Science, 25 ( 9 ), 817 – 821. https://doi.org/10.1016/0032-0633(77)90035-6 | |
dc.identifier.citedreference | Kim, S., Caldwell, J., Rivolo, A., Wagener, R., & Orton, G. ( 1985 ). Infrared polar brightening on Jupiter III. Spectrometry from the Voyager 1 IRIS experiment. Icarus, 64 ( 2 ), 233 – 248. https://doi.org/10.1016/0019-1035(85)90088-0 | |
dc.identifier.citedreference | Kim, S., Drossart, P., Caldwell, J., Maillard, J. P., Herbst, T., & Shure, M. ( 1991 ). Images of aurorae on Jupiter from H 3 + emission at 4 μm. Nature, 353 ( 6344 ), 536 – 539. https://doi.org/10.1038/353536a0 | |
dc.identifier.citedreference | Kim, S., Geballe, T., Seo, H., & Jim, J. ( 2009 ). Jupiter’s hydrocarbon polar brightening: Discovery of 3-micron line emission from south polar CH 4, C 2 H 2 and C 2 H 6. Icarus, 202 ( 1 ), 354 – 357. https://doi.org/10.1016/j.icarus.2009.03.020 | |
dc.working.doi | NO | en |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
Remediation of Harmful Language
The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.
Accessibility
If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.