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    Rights statement: An edited version of this paper was published by AGU. Copyright 2016 American Geophysical Union. Badman, S. V., et al. (2016), Weakening of Jupiter's main auroral emission during January 2014, Geophys. Res. Lett., 43, 988–997, doi:10.1002/2015GL067366. To view the published open abstract, go to http://dx.doi.org/10.1002/2015GL067366

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    Available under license: CC BY-NC: Creative Commons Attribution-NonCommercial 4.0 International License

  • Badman_et_al-2016-Geophysical_Research_Letters

    Rights statement: ©2016. 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.

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Weakening of Jupiter's main auroral emission during January 2014

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Weakening of Jupiter's main auroral emission during January 2014. / Badman, S.V.; Bonfond, B.; Fujimoto, M. et al.
In: Geophysical Research Letters, Vol. 43, No. 3, 16.02.2016, p. 988-997.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Badman, SV, Bonfond, B, Fujimoto, M, Gray, B, Kasaba, Y, Kasahara, S, Kimura, T, Melin, H, Nichols, JD, Steffl, AJ, Tao, C, Tsuchiya, F, Yamazaki, A, Yoneda, M, Yoshikawa, I & Yoshioka, K 2016, 'Weakening of Jupiter's main auroral emission during January 2014', Geophysical Research Letters, vol. 43, no. 3, pp. 988-997. https://doi.org/10.1002/2015GL067366

APA

Badman, S. V., Bonfond, B., Fujimoto, M., Gray, B., Kasaba, Y., Kasahara, S., Kimura, T., Melin, H., Nichols, J. D., Steffl, A. J., Tao, C., Tsuchiya, F., Yamazaki, A., Yoneda, M., Yoshikawa, I., & Yoshioka, K. (2016). Weakening of Jupiter's main auroral emission during January 2014. Geophysical Research Letters, 43(3), 988-997. https://doi.org/10.1002/2015GL067366

Vancouver

Badman SV, Bonfond B, Fujimoto M, Gray B, Kasaba Y, Kasahara S et al. Weakening of Jupiter's main auroral emission during January 2014. Geophysical Research Letters. 2016 Feb 16;43(3):988-997. Epub 2016 Feb 10. doi: 10.1002/2015GL067366

Author

Badman, S.V. ; Bonfond, B. ; Fujimoto, M. et al. / Weakening of Jupiter's main auroral emission during January 2014. In: Geophysical Research Letters. 2016 ; Vol. 43, No. 3. pp. 988-997.

Bibtex

@article{a1eaa2ec59f042cba01cbf941a284eb6,
title = "Weakening of Jupiter's main auroral emission during January 2014",
abstract = "In January 2014 Jupiter's FUV main auroral oval decreased its emitted power by 70% and shifted equatorward by ∼1°. Intense, low-latitude features were also detected. The decrease in emitted power is attributed to a decrease in auroral current density rather than electron energy. This could be caused by a decrease in the source electron density, an order of magnitude increase in the source electron thermal energy, or a combination of these. Both can be explained either by expansion of the magnetosphere or by an increase in the inward transport of hot plasma through the middle magnetosphere and its interchange with cold flux tubes moving outward. In the latter case the hot plasma could have increased the electron temperature in the source region and produced the intense, low-latitude features, while the increased cold plasma transport rate produced the shift of the main oval.",
author = "S.V. Badman and B. Bonfond and M. Fujimoto and Becky Gray and Y. Kasaba and S. Kasahara and T. Kimura and H. Melin and J.D. Nichols and A.J. Steffl and C. Tao and F. Tsuchiya and A. Yamazaki and M. Yoneda and I. Yoshikawa and K. Yoshioka",
note = "An edited version of this paper was published by AGU. Copyright 2016 American Geophysical Union. Badman, S. V., et al. (2016), Weakening of Jupiter's main auroral emission during January 2014, Geophys. Res. Lett., 43, 988–997, doi:10.1002/2015GL067366. To view the published open abstract, go to http://dx.doi.org/10.1002/2015GL067366",
year = "2016",
month = feb,
day = "16",
doi = "10.1002/2015GL067366",
language = "English",
volume = "43",
pages = "988--997",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "John Wiley & Sons, Ltd",
number = "3",

}

RIS

TY - JOUR

T1 - Weakening of Jupiter's main auroral emission during January 2014

AU - Badman, S.V.

AU - Bonfond, B.

AU - Fujimoto, M.

AU - Gray, Becky

AU - Kasaba, Y.

AU - Kasahara, S.

AU - Kimura, T.

AU - Melin, H.

AU - Nichols, J.D.

AU - Steffl, A.J.

AU - Tao, C.

AU - Tsuchiya, F.

AU - Yamazaki, A.

AU - Yoneda, M.

AU - Yoshikawa, I.

AU - Yoshioka, K.

N1 - An edited version of this paper was published by AGU. Copyright 2016 American Geophysical Union. Badman, S. V., et al. (2016), Weakening of Jupiter's main auroral emission during January 2014, Geophys. Res. Lett., 43, 988–997, doi:10.1002/2015GL067366. To view the published open abstract, go to http://dx.doi.org/10.1002/2015GL067366

PY - 2016/2/16

Y1 - 2016/2/16

N2 - In January 2014 Jupiter's FUV main auroral oval decreased its emitted power by 70% and shifted equatorward by ∼1°. Intense, low-latitude features were also detected. The decrease in emitted power is attributed to a decrease in auroral current density rather than electron energy. This could be caused by a decrease in the source electron density, an order of magnitude increase in the source electron thermal energy, or a combination of these. Both can be explained either by expansion of the magnetosphere or by an increase in the inward transport of hot plasma through the middle magnetosphere and its interchange with cold flux tubes moving outward. In the latter case the hot plasma could have increased the electron temperature in the source region and produced the intense, low-latitude features, while the increased cold plasma transport rate produced the shift of the main oval.

AB - In January 2014 Jupiter's FUV main auroral oval decreased its emitted power by 70% and shifted equatorward by ∼1°. Intense, low-latitude features were also detected. The decrease in emitted power is attributed to a decrease in auroral current density rather than electron energy. This could be caused by a decrease in the source electron density, an order of magnitude increase in the source electron thermal energy, or a combination of these. Both can be explained either by expansion of the magnetosphere or by an increase in the inward transport of hot plasma through the middle magnetosphere and its interchange with cold flux tubes moving outward. In the latter case the hot plasma could have increased the electron temperature in the source region and produced the intense, low-latitude features, while the increased cold plasma transport rate produced the shift of the main oval.

U2 - 10.1002/2015GL067366

DO - 10.1002/2015GL067366

M3 - Journal article

VL - 43

SP - 988

EP - 997

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - 3

ER -