Home > Research > Publications & Outputs > Response of Jupiter's auroras to conditions in ...

Research

Associated organisational unit

Electronic data

  • HSTJuno_v2.0

    Rights statement: Accepted for publication in Geophysical Research Letters. Copyright 2017 American Geophysical Union. Further reproduction or electronic distribution is not permitted.

    Accepted author manuscript, 3.24 MB, PDF document

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

  • Nichols_et_al-2017-Geophysical_Research_Letters

    Rights statement: ©2017. 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.

    Final published version, 5.35 MB, PDF document

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

Links

Text available via DOI:

View graph of relations

Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Published

Standard

Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno. / Nichols, J.D.; Badman, Sarah Victoria; Bagenal, F. et al.
In: Geophysical Research Letters, Vol. 44, No. 15, 16.08.2017, p. 7643-7652.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Nichols, JD, Badman, SV, Bagenal, F, Bolton, SJ, Bonfond, B, Bunce, E, Clarke, JT, Connerney, JEP, Cowley, SWH, Ebert, RW, Fujimoto, M, Gerard, JC, Gladstone, GR, Grodent, D, Kimura, T, Kurth, WS, Mauk, BH, Murakami, G, McComas, DJ, Orton, GS, Radioti, A, Stallard, T, Tao, C, Valek, PW, Wilson, R, Yamazaki, A & Yoshikawa, I 2017, 'Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno', Geophysical Research Letters, vol. 44, no. 15, pp. 7643-7652. https://doi.org/10.1002/2017GL073029

APA

Nichols, J. D., Badman, S. V., Bagenal, F., Bolton, S. J., Bonfond, B. ., Bunce, E., Clarke, J. T., Connerney, J. E. P., Cowley, S. W. H., Ebert, R. W., Fujimoto, M., Gerard, J. C., Gladstone, G. R., Grodent, D., Kimura, T., Kurth, W. S., Mauk, B. H., Murakami, G., McComas, D. J., ... Yoshikawa, I. (2017). Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno. Geophysical Research Letters, 44(15), 7643-7652. https://doi.org/10.1002/2017GL073029

Vancouver

Nichols JD, Badman SV, Bagenal F, Bolton SJ, Bonfond B, Bunce E et al. Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno. Geophysical Research Letters. 2017 Aug 16;44(15):7643-7652. Epub 2017 May 25. doi: 10.1002/2017GL073029

Author

Nichols, J.D. ; Badman, Sarah Victoria ; Bagenal, F. et al. / Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno. In: Geophysical Research Letters. 2017 ; Vol. 44, No. 15. pp. 7643-7652.

Bibtex

@article{e49307cd8d68456ea8a3853d8e0c4217,
title = "Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno",
abstract = "We present the first comparison of Jupiter's auroral morphology with an extended, continuous and complete set of near-Jupiter interplanetary data, revealing the response of Jupiter's auroras to the interplanetary conditions. We show that for ∼1-3 days following compression region onset the planet's main emission brightened. A duskside poleward region also brightened during compressions, as well as during shallow rarefaction conditions at the start of the program. The power emitted from the noon active region did not exhibit dependence on any interplanetary parameter, though the morphology typically differed between rarefactions and compressions. The auroras equatorward of the main emission brightened over ∼10 days following an interval of increased volcanic activity on Io. These results show that the dependence of Jupiter's magnetosphere and auroras on the interplanetary conditions are more diverse than previously thought.",
author = "J.D. Nichols and Badman, {Sarah Victoria} and F. Bagenal and Bolton, {S. J.} and Bonfond, {B. .} and Emma Bunce and Clarke, {J. T.} and Connerney, {J. E. P.} and Cowley, {S. W. H.} and Ebert, {R. W.} and M. Fujimoto and Gerard, {Jean Claude} and Gladstone, {G. R.} and Denis Grodent and T. Kimura and W.S. Kurth and Mauk, {Barry H.} and G. Murakami and McComas, {D. J.} and Orton, {G. S.} and Aikaterini Radioti and Tom Stallard and Chihiro Tao and P.W. Valek and R. Wilson and A. Yamazaki and I. Yoshikawa",
note = "Accepted for publication in Geophysical Research Letters. Copyright 2017 American Geophysical Union. Further reproduction or electronic distribution is not permitted. {\textcopyright}2017. 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.",
year = "2017",
month = aug,
day = "16",
doi = "10.1002/2017GL073029",
language = "English",
volume = "44",
pages = "7643--7652",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "John Wiley & Sons, Ltd",
number = "15",

}

RIS

TY - JOUR

T1 - Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

AU - Nichols, J.D.

AU - Badman, Sarah Victoria

AU - Bagenal, F.

AU - Bolton, S. J.

AU - Bonfond, B. .

AU - Bunce, Emma

AU - Clarke, J. T.

AU - Connerney, J. E. P.

AU - Cowley, S. W. H.

AU - Ebert, R. W.

AU - Fujimoto, M.

AU - Gerard, Jean Claude

AU - Gladstone, G. R.

AU - Grodent, Denis

AU - Kimura, T.

AU - Kurth, W.S.

AU - Mauk, Barry H.

AU - Murakami, G.

AU - McComas, D. J.

AU - Orton, G. S.

AU - Radioti, Aikaterini

AU - Stallard, Tom

AU - Tao, Chihiro

AU - Valek, P.W.

AU - Wilson, R.

AU - Yamazaki, A.

AU - Yoshikawa, I.

N1 - Accepted for publication in Geophysical Research Letters. Copyright 2017 American Geophysical Union. Further reproduction or electronic distribution is not permitted. ©2017. 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.

PY - 2017/8/16

Y1 - 2017/8/16

N2 - We present the first comparison of Jupiter's auroral morphology with an extended, continuous and complete set of near-Jupiter interplanetary data, revealing the response of Jupiter's auroras to the interplanetary conditions. We show that for ∼1-3 days following compression region onset the planet's main emission brightened. A duskside poleward region also brightened during compressions, as well as during shallow rarefaction conditions at the start of the program. The power emitted from the noon active region did not exhibit dependence on any interplanetary parameter, though the morphology typically differed between rarefactions and compressions. The auroras equatorward of the main emission brightened over ∼10 days following an interval of increased volcanic activity on Io. These results show that the dependence of Jupiter's magnetosphere and auroras on the interplanetary conditions are more diverse than previously thought.

AB - We present the first comparison of Jupiter's auroral morphology with an extended, continuous and complete set of near-Jupiter interplanetary data, revealing the response of Jupiter's auroras to the interplanetary conditions. We show that for ∼1-3 days following compression region onset the planet's main emission brightened. A duskside poleward region also brightened during compressions, as well as during shallow rarefaction conditions at the start of the program. The power emitted from the noon active region did not exhibit dependence on any interplanetary parameter, though the morphology typically differed between rarefactions and compressions. The auroras equatorward of the main emission brightened over ∼10 days following an interval of increased volcanic activity on Io. These results show that the dependence of Jupiter's magnetosphere and auroras on the interplanetary conditions are more diverse than previously thought.

U2 - 10.1002/2017GL073029

DO - 10.1002/2017GL073029

M3 - Journal article

VL - 44

SP - 7643

EP - 7652

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - 15

ER -