Journal
GEOPHYSICAL RESEARCH LETTERS
Volume 44, Issue 16, Pages 8107-8112Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1002/2017GL073175
Keywords
Hot flow anomaly; Jupiter; Bow shock; Juno
Categories
Funding
- NASA's Juno mission
- STFC [ST/P000541/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/P000541/1] Funding Source: researchfish
Ask authors/readers for more resources
A Hot Flow Anomaly (HFA) is created when an interplanetary current sheet interacts with a planetary bow shock. Previous studies have reported observing HFAs at Earth, Mercury, Venus, Mars, and Saturn. During Juno's approach to Jupiter, a number of its instruments operated in the solar wind. Prior to crossing into Jupiter's magnetosphere, Juno observed an HFA at Jupiter for the first time. This Jovian HFA shares most of the characteristics of HFAs seen at other planets. The notable exception is that the Jovian HFA is significantly larger than any HFA seen before. With an apparent size greater than 2x10(6)km the Jovian HFA is orders of magnitude larger than those seen at the other planets. By comparing the size of the HFAs at the other planets with the Jovian HFA, we conclude that HFAs size scales with the size of planetary bow shocks that the interplanetary current sheet interacts with.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available