Drew A. Coffin, Paul Withers, Omakshi Agiwal, Dustin Buccino, Marzia Parisi, Ryan S. Caruso, Andrea Caruso, Luis Gomez Casajus, Edoardo Gramigna, Paolo Tortora, Marco Zannoni, Jack Hunter Waite, Paul Steffes, Sushil Atreya, Scott Bolton
{"title":"Juno-Derived Electron Density Profiles of the High-Latitude Jovian Ionosphere","authors":"Drew A. Coffin, Paul Withers, Omakshi Agiwal, Dustin Buccino, Marzia Parisi, Ryan S. Caruso, Andrea Caruso, Luis Gomez Casajus, Edoardo Gramigna, Paolo Tortora, Marco Zannoni, Jack Hunter Waite, Paul Steffes, Sushil Atreya, Scott Bolton","doi":"10.1029/2025JA033754","DOIUrl":null,"url":null,"abstract":"<p>The magnetosphere of Jupiter is an excellent natural laboratory for plasma dynamics due to its strength and internal plasma source. However, a complication in understanding the flow of energy through the system is the closure of the driving current systems within the chaotic high-latitude ionosphere of Jupiter, a region that has been poorly surveyed. The polar orbit of the Juno spacecraft permits for the first time multiple observations of the high- and mid-latitude ionosphere through the radio occultation technique. This paper presents derived electron density profiles from four such occultations. Seven profiles, four ingress and three egress, all sample the dawn limb but at a range of magnetic latitudes, including an ingress profile within <span></span><math>\n <semantics>\n <mrow>\n <msup>\n <mn>5</mn>\n <mi>o</mi>\n </msup>\n </mrow>\n <annotation> ${5}^{o}$</annotation>\n </semantics></math> of the main oval that is consistent with a response to high-energy electron influx. These profiles demonstrate variability in peak densities, peak altitude, and even the number of layers present. This high level of variability in Jupiter's high-latitude ionosphere suggests a complex network of current closure with high temporal variability.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 6","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2025-06-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2025JA033754","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
The magnetosphere of Jupiter is an excellent natural laboratory for plasma dynamics due to its strength and internal plasma source. However, a complication in understanding the flow of energy through the system is the closure of the driving current systems within the chaotic high-latitude ionosphere of Jupiter, a region that has been poorly surveyed. The polar orbit of the Juno spacecraft permits for the first time multiple observations of the high- and mid-latitude ionosphere through the radio occultation technique. This paper presents derived electron density profiles from four such occultations. Seven profiles, four ingress and three egress, all sample the dawn limb but at a range of magnetic latitudes, including an ingress profile within of the main oval that is consistent with a response to high-energy electron influx. These profiles demonstrate variability in peak densities, peak altitude, and even the number of layers present. This high level of variability in Jupiter's high-latitude ionosphere suggests a complex network of current closure with high temporal variability.