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Residual Study: Testing Jupiter Atmosphere Models Against Juno MWR Observations

Zhang, Zhimeng and Adumitroaie, Virgil and Allison, Michael and Arballo, John and Atreya, Sushil and Bjoraker, Gordon and Bolton, Scott and Brown, Shannon and Fletcher, Leigh N. and Guillot, Tristan and Gulkis, Samuel and Hodges, Amoree and Ingersoll, Andrew and Janssen, Michael and Levin, Steven and Li, Cheng and Li, Liming and Lunine, Jonathan and Misra, Sidharth and Orton, Glenn and Oyafuso, Fabiano and Steffes, Paul and Wong, Michael H. (2020) Residual Study: Testing Jupiter Atmosphere Models Against Juno MWR Observations. Earth and Space Science, 7 (9). Art. No. e2020EA001229. ISSN 2333-5084. https://resolver.caltech.edu/CaltechAUTHORS:20200818-104028139

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Abstract

The Juno spacecraft provides unique close‐up views of Jupiter underneath the synchrotron radiation belts while circling Jupiter in its 53‐day orbits. The microwave radiometer (MWR) onboard measures Jupiter thermal radiation at wavelengths between 1.37 and 50 cm, penetrating the atmosphere to a pressure of a few hundred bars and greater. The mission provides the first measurements of Jupiter's deep atmosphere, down to ~250 bars in pressure, constraining the vertical distributions of its kinetic temperature and constituents. As a result, vertical structure models of Jupiter's atmosphere may now be tested by comparison with MWR data. Taking into account the MWR beam patterns and observation geometries, we test several published Jupiter atmospheric models against MWR data. Our residual analysis confirms Li et al.'s (2017, https://doi.org/10.1002/2017GL073159) result that ammonia depletion persists down to 50–60 bars where ground‐based Very Large Array was not able to observe. We also present an extension of the study that iteratively improves the input model and generates Jupiter brightness temperature maps which best match the MWR data. A feature of Juno's north‐to‐south scanning approach is that latitudinal structure is more easily obtained than longitudinal, and the creation of optimum two‐dimensional maps is addressed in this approach.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1029/2020ea001229DOIArticle
https://pds-atmospheres.nmsu.edu/data_and_services/atmospheres_data/JUNO/microwave.htmlRelated ItemData
https://pds-atmospheres.nmsu.edu/PDS/data/jnomwr_1100/data_calibratedRelated ItemData
http://doi.org/10.5281/zenodo.3936065DOIData
ORCID:
AuthorORCID
Zhang, Zhimeng0000-0002-1558-4948
Adumitroaie, Virgil0000-0001-7239-0069
Allison, Michael0000-0001-9841-193X
Atreya, Sushil0000-0002-1972-1815
Bolton, Scott0000-0002-9115-0789
Brown, Shannon0000-0002-7566-8537
Fletcher, Leigh N.0000-0001-5834-9588
Guillot, Tristan0000-0002-7188-8428
Gulkis, Samuel0000-0002-4480-3628
Hodges, Amoree0000-0002-4894-5826
Ingersoll, Andrew0000-0002-2035-9198
Janssen, Michael0000-0001-5476-731X
Levin, Steven0000-0003-2242-5459
Li, Cheng0000-0002-8280-3119
Li, Liming0000-0002-5257-9849
Lunine, Jonathan0000-0003-2279-4131
Misra, Sidharth0000-0003-1738-6635
Orton, Glenn0000-0001-7871-2823
Oyafuso, Fabiano0000-0002-8862-8737
Steffes, Paul0000-0003-3962-8957
Wong, Michael H.0000-0003-2804-5086
Additional Information:© 2020 The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. Issue Online: 19 September 2020; Version of Record online: 19 September 2020; Accepted manuscript online: 06 August 2020; Manuscript accepted: 18 July 2020; Manuscript revised: 08 July 2020; Manuscript received: 14 April 2020. This work is supported by Juno mission under 699048X. Data Availability Statement: The Juno MWR observations used in this analysis work are available through the Planetary Data System Atmospheres Node. Data are stored in ASCII tables with supporting documentation (https://pds-atmospheres.nmsu.edu/data_and_services/atmospheres_data/JUNO/microwave.html). Data files can be found online (https://pds-atmospheres.nmsu.edu/PDS/data/jnomwr_1100/data_calibrated/). All data sets for this research are available in the citation reference: Zhang, Zhimeng, Adumitroaie, Virgil, Allison, Michael, Arballo, John, Atreya, Sushil, Bjoraker, Gordon, … Wong, Michael. (2020). Dataset for Residual Study: Testing Jupiter Atmosphere Models Against Juno MWR Observations [Data set]. Zenodo. http://doi.org/10.5281/zenodo.3936065.
Funders:
Funding AgencyGrant Number
NASA699048X
Subject Keywords:Jupiter; Juno; Atmosphere; Giant planets; Microwave Radiometer
Issue or Number:9
Record Number:CaltechAUTHORS:20200818-104028139
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200818-104028139
Official Citation:Zhang, Z., Adumitroaie, V., Allison, M., Arballo, J., Atreya, S., & Bjoraker, G., et al. (2020). Residual study: Testing Jupiter atmosphere models against Juno MWR observations. Earth and Space Science, 7, e2020EA001229. https://doi.org/10.1029/2020EA001229
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104996
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:18 Aug 2020 18:11
Last Modified:23 Sep 2020 16:16

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