Play all audios:
ABSTRACT The exchange of energy and momentum between the Earth’s upper atmosphere and ionosphere, and its space environment (magnetosphere) is regulated by electric currents (called
Birkeland currents) flowing along magnetic field lines that connect these two regions of space1. The associated electric currents flow towards and away from each pole primarily in two
concentric conical sheets2. It has been expected that powerful sheets of magnetic-field-aligned electric currents would be found in association with the bright Jovian auroras3. The Juno
spacecraft is well positioned to explore Jupiter’s polar magnetosphere and sample Birkeland or field-aligned currents and particle distributions. Since July 2016, Juno has maintained a
near-polar orbit, passing over both polar regions every 53 days. From this vantage point, Juno’s complement of science instruments gathers in situ observations of magnetospheric particles
and fields while its remote-sensing infrared and ultraviolet spectrographs and imagers map auroral emissions4. Here we present an extensive analysis of magnetic field perturbations measured
during Juno’s transits of Jupiter’s polar regions, and thereby demonstrate Birkeland currents associated with Jupiter’s auroral emissions. We characterize the magnitude and spatial extent of
the currents and we find that they are weaker than anticipated and filamentary in nature. A significant asymmetry is observed between the field perturbations and the current associated with
the northern and the southern auroras. Access through your institution Buy or subscribe This is a preview of subscription content, access via your institution ACCESS OPTIONS Access through
your institution Access Nature and 54 other Nature Portfolio journals Get Nature+, our best-value online-access subscription $32.99 / 30 days cancel any time Learn more Subscribe to this
journal Receive 12 digital issues and online access to articles $119.00 per year only $9.92 per issue Learn more Buy this article * Purchase on SpringerLink * Instant access to full article
PDF Buy now Prices may be subject to local taxes which are calculated during checkout ADDITIONAL ACCESS OPTIONS: * Log in * Learn about institutional subscriptions * Read our FAQs * Contact
customer support SIMILAR CONTENT BEING VIEWED BY OTHERS TWO DISTINCT CURRENT SYSTEMS IN THE IONOSPHERE OF MARS Article Open access 09 November 2024 IN SITU EVIDENCE OF THE MAGNETOSPHERIC
CUSP OF JUPITER FROM JUNO SPACECRAFT MEASUREMENTS Article Open access 18 July 2024 ENERGETIC NEUTRAL ATOM IMAGING REVEALS NEARLY 11-YEAR CYCLE OF THE RING CURRENT OF SATURN Article Open
access 05 December 2024 DATA AVAILABILITY The Juno magnetometer data used in this study will be made available through the NASA Planetary Data System (https://pds.nasa.gov) in accordance
with NASA policy. CHANGE HISTORY * _ 14 OCTOBER 2019 An amendment to this paper has been published and can be accessed via a link at the top of the paper. _ REFERENCES * Birkeland, K. _The
Norwegian Aurora Polaris Expedition 1902–1903_ Vol. 1 (H. Aschelhoug & Co., 1908). * Potemra, T. A. Birkeland currents in the Earth’s magnetosphere. _Astrophys. Space Sci._ 144, 155–169
(1988). ADS Google Scholar * Connerney, J. E. P. et al. Jupiter’s magnetosphere and aurorae observed by the Juno spacecraft during its first polar orbits. _Science_ 356, 826–832 (2017).
Article ADS Google Scholar * Bagenal, F. et al. Magnetospheric science objectives of the Juno mission. _Space Sci. Rev._ 213, 219–287 (2017). Article ADS Google Scholar * Gladstone, G.
R. et al. The ultraviolet spectrograph on NASA’s Juno mission. _Space Sci. Rev._ 213, 447–473 (2017). Article ADS Google Scholar * Bonfond, B. et al. Morphology of the UV aurorae Jupiter
during Juno’s first perijove observations. _Geophys. Res. Lett._ 44, 4463–4471 (2017). Article ADS Google Scholar * Connerney, J. E. P. et al. A new model of Jupiter’s magnetic field
from Juno’s first nine orbits. _Geophys. Res. Lett._ 45, 2590–2596 (2018). Article ADS Google Scholar * Connerney, J. E. P., Acua, M. H. & Ness, N. F. Modeling the Jovian current
sheet and inner magnetosphere. _J. Geophys. Res. Space Phys._ 86, 8370–8384 (1981). Article ADS Google Scholar * Lühr, H., Warnecke, F., Jórg, K. A. & Rother, M. An algorithm for
estimating field-aligned currents from single spacecraft magnetic field measurements: a diagnostic tool applied to Freja satellite data. _IEEE Trans. Geosci. Remote Sens._ 34, 1369–1376
(1996). Article ADS Google Scholar * Hoffman, R. A., Fujii, R. & Sugiura, M. Characteristics of the field-aligned current system in the nighttime sector during auroral substorms. _J.
Geophys. Res. Space Phys._ 99, 21303–21325 (1994). Article ADS Google Scholar * Kurth, W. S. et al. The Juno waves investigation. _Space Sci. Rev._ 213, 347–392 (2017). Article ADS
Google Scholar * McComas, D. J. et al. The Jovian Auroral Distributions Experiment (JADE) on the Juno mission to Jupiter. _Space Sci. Rev._ 213, 547–643 (2017). Article ADS Google Scholar
* Mauk, B. H. et al. The Jupiter Energetic Particle Detector Instrument (JEDI) investigation for the Juno mission. _Space Sci. Rev._ 213, 289–346 (2017). Article ADS Google Scholar *
Chaston, C. C. et al. The turbulent Alfvénic aurora. _Phys. Rev. Lett._ 100, 175003 (2008). Article ADS Google Scholar * Mauk, B. H. et al. Discrete and broadband electron acceleration in
Jupiter’s powerful aurora. _Nature_ 549, 66–69 (2017). Article ADS Google Scholar * Saur, J., Annick, P. & William, M. H. An acceleration mechanism for the generation of the main
auroral oval on Jupiter. _Geophys. Res. Lett._ 30, 1260 (2003). Article ADS Google Scholar * Saur, J. et al. Wave-particle interaction of Alfvén waves in Jupiter’s magnetosphere: auroral
and magnetospheric particle acceleration: wave-particle interaction in Jupiter’s magnetosphere. _J. Geophys. Res. Space Phys._ 123, 9560–9573 (2018). Article ADS Google Scholar * Mauk, B.
H. et al. Diverse electron and ion acceleration characteristics observed over Jupiter’s main aurora. _Geophys. Res. Lett._ 45, 1277–1285 (2018). Article ADS Google Scholar * Chaston, C.
et al. Turbulent heating and cross-field transport near the magnetopause from THEMIS. _Geophys. Res. Lett._ 35, L17S08 (2008). Article Google Scholar * Moore, K. M. et al. A complex dynamo
inferred from the hemispheric dichotomy of Jupiter’s magnetic field. _Nature_ 561, 76–78 (2018). Article ADS Google Scholar * Parish, J. L., Goertz, C. K. & Thomsen, M. F. Azimuthal
magnetic field at Jupiter. _J. Geophys. Res._ 85, 4152–4156 (1980). Article ADS Google Scholar * Connerney, J. E. P. Comment on ‘Azimuthal magnetic field at Jupiter’ by J. L. Parish, C.
K. Goertz, and M. F. Thomsen. _J. Geophys. Res. Space Phys._ 86, 7796–7797 (1981). Article ADS Google Scholar * Khurana, K. K. Influence of solar wind on Jupiter’s magnetosphere deduced
from currents in the equatorial plane. _J. Geophys. Res. Space Phys._ 106, 25999–26016 (2001). Article ADS Google Scholar * Cowley, S. & Bunce, E. Origin of the main auroral oval in
Jupiter’s coupled magnetosphere–ionosphere system. _Planet. Space Sci._ 49, 1067–1088 (2001). Article ADS Google Scholar * Ray, L. C., Ergun, R. E., Delamere, P. A. & Bagenal, F.
Magnetosphere–ionosphere coupling at Jupiter: effect of field-aligned potentials on angular momentum transport. _J. Geophys. Res. Space Phys._ 115, A09211 (2010). ADS Google Scholar * Tao,
C., Fujiwara, H. & Kasaba, Y. Neutral wind control of the Jovian magnetosphere–ionosphere current system. _J. Geophys. Res. Space Phys._ 114, A08307 (2009). ADS Google Scholar *
Iijima, T. & Potemra, T. A. Large-scale characteristics of field-aligned currents associated with substorms. _J. Geophys. Res. Space Phys._ 83, 599–615 (1978). Article ADS Google
Scholar * Moen, J. & Brekke, A. On the importance of ion composition to conductivities in the auroral ionosphere. _J. Geophys. Res. Space Phys._ 95, 10687–10693 (1990). Article ADS
Google Scholar * Garcia, D. Robust smoothing of gridded data in one and higher dimensions with missing values. _Comput. Stat. Data Anal._ 54, 1167–1178 (2010). Article MathSciNet Google
Scholar * Connerney, J. E. P. et al. The Juno magnetic field investigation. _Space Sci. Rev._ 213, 39–138 (2017). Article ADS Google Scholar * Lam, H. A. et al. A baseline spectroscopic
study of the infrared auroras of Jupiter. _Icarus_ 127, 379–393 (1997). Article ADS Google Scholar * Hinson, D. P. et al. Jupiter’s ionosphere: results from the first Galileo radio
occultation experiment. _Geophys. Res. Lett._ 24, 2107–2110 (1997). Article ADS Google Scholar * Ridley, A. J. Effects of seasonal changes in the ionospheric conductances on
magnetospheric field-aligned currents. _Geophys. Res. Lett._ 34, L05101 (2007). Article ADS Google Scholar * Dessler, A. J. in _Physics Of The Jovian Magnetosphere_ (ed. Dessler, A. J.)
498–504 (Cambridge Planetary Science Old, 1983). Download references ACKNOWLEDGEMENTS S.K. thanks F. Bagenal for the motivation and valuable scientific discussions in relation to this paper.
All authors acknowledge support from the Juno project. E.J.B. was supported by STFC grant ST/N000749/1 and a Royal Society Wolfson Research Merit Award. AUTHOR INFORMATION AUTHORS AND
AFFILIATIONS * NASA Goddard Space Flight Center, Greenbelt, MD, USA Stavros Kotsiaros, John E. P. Connerney, Daniel J. Gershman & Yasmina M. Martos * University of Maryland College Park,
College Park, MD, USA Stavros Kotsiaros & Yasmina M. Martos * Space Research Corporation, Annapolis, MD, USA John E. P. Connerney * Johns Hopkins University Applied Physics Laboratory,
Laurel, MD, USA George Clark & Barry H. Mauk * Southwest Research Institute, San Antonio, TX, USA Frederic Allegrini, G. Randall Gladstone, Thomas K. Greathouse & Scott J. Bolton *
Department of Physics and Astronomy, University of Texas at San Antonio, San Antonio, TX, USA Frederic Allegrini & G. Randall Gladstone * Department of Physics and Astronomy, University
of Iowa, Iowa City, IA, USA William S. Kurth * Universität zu Köln, Institut für Geophysik und Meteorologie, Cologne, Germany Joachim Saur * Department of Physics and Astronomy, University
of Leicester, Leicester, UK Emma J. Bunce * Jet Propulsion Laboratory, Pasadena, CA, USA Steven M. Levin Authors * Stavros Kotsiaros View author publications You can also search for this
author inPubMed Google Scholar * John E. P. Connerney View author publications You can also search for this author inPubMed Google Scholar * George Clark View author publications You can
also search for this author inPubMed Google Scholar * Frederic Allegrini View author publications You can also search for this author inPubMed Google Scholar * G. Randall Gladstone View
author publications You can also search for this author inPubMed Google Scholar * William S. Kurth View author publications You can also search for this author inPubMed Google Scholar *
Barry H. Mauk View author publications You can also search for this author inPubMed Google Scholar * Joachim Saur View author publications You can also search for this author inPubMed Google
Scholar * Emma J. Bunce View author publications You can also search for this author inPubMed Google Scholar * Daniel J. Gershman View author publications You can also search for this
author inPubMed Google Scholar * Yasmina M. Martos View author publications You can also search for this author inPubMed Google Scholar * Thomas K. Greathouse View author publications You
can also search for this author inPubMed Google Scholar * Scott J. Bolton View author publications You can also search for this author inPubMed Google Scholar * Steven M. Levin View author
publications You can also search for this author inPubMed Google Scholar CONTRIBUTIONS S.K. wrote the manuscript and performed the magnetic field data analysis. J.E.P.C. contributed to the
discussions of the data analysis and assisted with the writing of the manuscript. G.C. and F.A. performed the data analysis of the JEDI and JADE instruments and contributed to Fig. 3 of the
manuscript. G.R.G. performed the data analysis of the UVS instrument and contributed to Fig. 1 of the manuscript. W.S.K. performed the data analysis of the Waves instrument and contributed
to Supplementary Fig. 2 of the manuscript. D.J.G. contributed to the magnetic field data calibration and the discussions of the data analysis. B.H.M., T.K.G and Y.M.M. contributed to the
discussions of the data analysis. J.S. and E.J.B. contributed to the discussions of the physics of the Birkeland currents and the data analysis. S.J.B. is the principal investigator of the
mission and S.M.L. is the project scientist of the mission. CORRESPONDING AUTHOR Correspondence to Stavros Kotsiaros. ETHICS DECLARATIONS COMPETING INTERESTS The authors declare no competing
interests. ADDITIONAL INFORMATION PUBLISHER’S NOTE: Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations. SUPPLEMENTARY
INFORMATION SUPPLEMENTARY INFORMATION Supplementary Figs. 1–3 and Supplementary reference 1. RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Kotsiaros,
S., Connerney, J.E.P., Clark, G. _et al._ Birkeland currents in Jupiter’s magnetosphere observed by the polar-orbiting Juno spacecraft. _Nat Astron_ 3, 904–909 (2019).
https://doi.org/10.1038/s41550-019-0819-7 Download citation * Received: 06 January 2019 * Accepted: 15 May 2019 * Published: 08 July 2019 * Issue Date: October 2019 * DOI:
https://doi.org/10.1038/s41550-019-0819-7 SHARE THIS ARTICLE Anyone you share the following link with will be able to read this content: Get shareable link Sorry, a shareable link is not
currently available for this article. Copy to clipboard Provided by the Springer Nature SharedIt content-sharing initiative