ISSI  |  NSSC  
 
 
Home About us Program Publications Outreach Visitors Info Contact Us
Location: Home>News
SPACE SCIENCE RESEARCH
Submit a proposal
PROGRAM
ISSI-BJ Activities
Online Seminars
Forums
International Teams
Workshops
Working Groups
Visiting Scientists
Space Science School
MEDIA
ISSI-BJ in the media
Press Kit
News
The Earth-Like "Dawn Storm" Auroras of Jupiter 


Credit: NASA/JPL-Caltech/SwRI/UVS/STScI/MODIS/WIC/IMAGE/ULiège

Some members of the ISSI-BJ International Team on "The morphology of auroras at Earth and giant planets: characteristics and their magnetospheric implications", led by Bertrand Bonfond (University of Liège) and Yao Zhonghua (University of Liège), recently made a ground-breaking discovery, whose results were published on AGU Advances: 
Bonfond, B., Yao, Z. H., Gladstone, G. R., Grodent, D., Gérard, J.-C., Matar, J., et al. (2021). Are dawn storms Jupiter's auroral substorms? AGU Advances, 2, e2020AV000275.

The article reports on the imaging of all development stages of spectacular auroral events at Jupiter, the so-called dawn storms. The observations show surprising similarities with auroral substorms at Earth, which are "..auroral events stemming from explosive magnetospheric reconfigurations."


When we looked at the whole dawn storm sequence, we couldn’t help but notice that the dawn storm auroras at Jupiter are very similar to a type of terrestrial auroras called substorms
Yao Zhonghua, University of Liège


 

Abstract 

"Dawn storms are among the brightest events in the Jovian aurorae. Up to now, they had only been observed from Earth-based observatories, only showing the Sun-facing side of the planet. Here, we show for the first time global views of the phenomenon, from its initiation to its end and from the nightside of the aurora onto the dayside. Based on Juno's first 20 orbits, some patterns now emerge. Small short-lived spots are often seen a couple of hours before the main emission starts to brighten and evolve from a straight arc to a more irregular one in the midnight sector. As the whole feature rotates dawn-ward, the arc then separates into two arcs with a central initially void region that is progressively filled with emissions. A gap in longitude then often forms before the whole feature dims. Finally, it transforms into an equatorward-moving patch of auroral emissions associated with plasma injection signatures. Some dawn storms remain weak and never fully develop. We also found cases of successive dawn storms within a few hours. Dawn storms thus share many fundamental features with the auroral signatures of the substorms at Earth, despite the substantial differences between the dynamics of the magnetosphere at the two planets."


The article is open-access, download it here:

https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2020AV000275


Watch the video here:

https://news.agu.org/press-release/jupiters-dawn-storm-auroras-are-surprisingly-earth-like-video/


Citation

Bonfond, B., Yao, Z. H., Gladstone, G. R., Grodent, D., Gérard, J.-C., Matar, J., et al. (2021). Are dawn storms Jupiter's auroral substorms? AGU Advances, 2, e2020AV000275.


Congratulations to Prof. Yao Zhonghua and his team!

 

 


Follow ISSI-BJ on Wechat or subscribe to the ISSI-BJ Newsletter!


 


相关附件
相关文档
CALENDAR
Upcoming Events
Message from the ISSI-BJ Executive Director
Announcements
Copyright © International Space Science Institute - Beijing
Address: No.1 Nanertiao, Zhongguancun, 100190 Haidian District, Beijing, China
Telephone: +86-10-62582811 - info@issibj.ac.cn
Wechat: ISSIBJ      Facebook: issibj       Linkedin: ISSI-BJ     Twitter: ISSIBeijing