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Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini

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Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini. / Guo, R.L.; Yao, Z.H.; Sergis, N. et al.
In: Astrophysical Journal Letters, Vol. 884, No. 1, 14, 10.10.2019.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Guo, RL, Yao, ZH, Sergis, N, Wei, Y, Xu, XJ, Coates, AJ, Delamere, PA, Roussos, E, Arridge, CS, Waite, JH, Krupp, N, Mitchell, D, Burch, J, Dougherty, MK & Wan, WX 2019, 'Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini', Astrophysical Journal Letters, vol. 884, no. 1, 14. https://doi.org/10.3847/2041-8213/ab4429

APA

Guo, R. L., Yao, Z. H., Sergis, N., Wei, Y., Xu, X. J., Coates, A. J., Delamere, P. A., Roussos, E., Arridge, C. S., Waite, J. H., Krupp, N., Mitchell, D., Burch, J., Dougherty, M. K., & Wan, W. X. (2019). Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini. Astrophysical Journal Letters, 884(1), Article 14. https://doi.org/10.3847/2041-8213/ab4429

Vancouver

Guo RL, Yao ZH, Sergis N, Wei Y, Xu XJ, Coates AJ et al. Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini. Astrophysical Journal Letters. 2019 Oct 10;884(1):14. Epub 2019 Oct 7. doi: 10.3847/2041-8213/ab4429

Author

Guo, R.L. ; Yao, Z.H. ; Sergis, N. et al. / Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini. In: Astrophysical Journal Letters. 2019 ; Vol. 884, No. 1.

Bibtex

@article{55749c96b217468ea1cd9129627b5266,
title = "Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini",
abstract = "The internal mass source from the icy moon Enceladus in Saturn?s rapidly rotating magnetosphere drives electromagnetic dynamics in multiple spatial and temporal scales. The distribution and circulation of the internal plasma and associated energy are thus crucial in understanding Saturn?s magnetospheric environment. Magnetic reconnection is one of the key processes in driving plasma and energy transport in the magnetosphere, and also a fundamental plasma process in energizing charged particles. Recent works suggested that reconnection driven by Saturn?s rapid rotation might appear as a chain of microscale structures, named drizzle-like reconnection. The drizzle-like reconnection could exist not only in the nightside magnetodisk, but also in the dayside magnetodisk. Here, using in situ measurements from the Cassini spacecraft, we report multiple reconnection sites that were successively detected during a time interval longer than one rotation period. The time separation between two adjacently detected reconnection sites can be much less than one rotation period, implying that the reconnection processes are likely small-scale, or frequently repetitive. The spatial distribution of the identified long-standing multiple small reconnection site sequences shows no significant preference on local times. We propose that the small reconnection sites discussed in this Letter are rotationally driven and rotate with the magnetosphere. Since the reconnection process on Saturn can be long-durational, the rotational regime can cause these small-scale reconnection sites to spread to all local times, resulting in global release of energy and mass from the magnetosphere.",
author = "R.L. Guo and Z.H. Yao and N. Sergis and Y. Wei and X.J. Xu and A.J. Coates and P.A. Delamere and E. Roussos and C.S. Arridge and J.H. Waite and N. Krupp and D. Mitchell and J. Burch and M.K. Dougherty and W.X. Wan",
year = "2019",
month = oct,
day = "10",
doi = "10.3847/2041-8213/ab4429",
language = "English",
volume = "884",
journal = "Astrophysical Journal Letters",
issn = "2041-8205",
publisher = "IOP Publishing Ltd",
number = "1",

}

RIS

TY - JOUR

T1 - Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini

AU - Guo, R.L.

AU - Yao, Z.H.

AU - Sergis, N.

AU - Wei, Y.

AU - Xu, X.J.

AU - Coates, A.J.

AU - Delamere, P.A.

AU - Roussos, E.

AU - Arridge, C.S.

AU - Waite, J.H.

AU - Krupp, N.

AU - Mitchell, D.

AU - Burch, J.

AU - Dougherty, M.K.

AU - Wan, W.X.

PY - 2019/10/10

Y1 - 2019/10/10

N2 - The internal mass source from the icy moon Enceladus in Saturn?s rapidly rotating magnetosphere drives electromagnetic dynamics in multiple spatial and temporal scales. The distribution and circulation of the internal plasma and associated energy are thus crucial in understanding Saturn?s magnetospheric environment. Magnetic reconnection is one of the key processes in driving plasma and energy transport in the magnetosphere, and also a fundamental plasma process in energizing charged particles. Recent works suggested that reconnection driven by Saturn?s rapid rotation might appear as a chain of microscale structures, named drizzle-like reconnection. The drizzle-like reconnection could exist not only in the nightside magnetodisk, but also in the dayside magnetodisk. Here, using in situ measurements from the Cassini spacecraft, we report multiple reconnection sites that were successively detected during a time interval longer than one rotation period. The time separation between two adjacently detected reconnection sites can be much less than one rotation period, implying that the reconnection processes are likely small-scale, or frequently repetitive. The spatial distribution of the identified long-standing multiple small reconnection site sequences shows no significant preference on local times. We propose that the small reconnection sites discussed in this Letter are rotationally driven and rotate with the magnetosphere. Since the reconnection process on Saturn can be long-durational, the rotational regime can cause these small-scale reconnection sites to spread to all local times, resulting in global release of energy and mass from the magnetosphere.

AB - The internal mass source from the icy moon Enceladus in Saturn?s rapidly rotating magnetosphere drives electromagnetic dynamics in multiple spatial and temporal scales. The distribution and circulation of the internal plasma and associated energy are thus crucial in understanding Saturn?s magnetospheric environment. Magnetic reconnection is one of the key processes in driving plasma and energy transport in the magnetosphere, and also a fundamental plasma process in energizing charged particles. Recent works suggested that reconnection driven by Saturn?s rapid rotation might appear as a chain of microscale structures, named drizzle-like reconnection. The drizzle-like reconnection could exist not only in the nightside magnetodisk, but also in the dayside magnetodisk. Here, using in situ measurements from the Cassini spacecraft, we report multiple reconnection sites that were successively detected during a time interval longer than one rotation period. The time separation between two adjacently detected reconnection sites can be much less than one rotation period, implying that the reconnection processes are likely small-scale, or frequently repetitive. The spatial distribution of the identified long-standing multiple small reconnection site sequences shows no significant preference on local times. We propose that the small reconnection sites discussed in this Letter are rotationally driven and rotate with the magnetosphere. Since the reconnection process on Saturn can be long-durational, the rotational regime can cause these small-scale reconnection sites to spread to all local times, resulting in global release of energy and mass from the magnetosphere.

U2 - 10.3847/2041-8213/ab4429

DO - 10.3847/2041-8213/ab4429

M3 - Journal article

VL - 884

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

SN - 2041-8205

IS - 1

M1 - 14

ER -