A. Santos, N. Achilleos, D. Millas, W. Dunn, P. Guio, C. S. Arridge
{"title":"Characterizing the Magnetic and Plasma Environment Upstream of Ganymede","authors":"A. Santos, N. Achilleos, D. Millas, W. Dunn, P. Guio, C. S. Arridge","doi":"10.1029/2024JA032689","DOIUrl":null,"url":null,"abstract":"<p>We present an application of the latest UCL-AGA magnetodisc model (MDISC) to the study of the magnetic and plasma conditions in the near-Ganymede space. By doing this, we provide a comparison with measurements from Juno's most recent flyby of the Jovian moon, perijove 34 (PJ34). We find good agreement between the model results and the magnetometer data, pointing toward a hot plasma index value <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>K</mi>\n <mi>h</mi>\n </msub>\n <mo>=</mo>\n </mrow>\n <annotation> ${K}_{h}=$</annotation>\n </semantics></math> (2.719<span></span><math>\n <semantics>\n <mrow>\n <mo>±</mo>\n </mrow>\n <annotation> $\\pm $</annotation>\n </semantics></math>0.024)<span></span><math>\n <semantics>\n <mrow>\n <mo>×</mo>\n </mrow>\n <annotation> ${\\times} $</annotation>\n </semantics></math>10<sup>7</sup> Pa m T<sup>−1</sup> and an effective magnetodisc radius <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>r</mi>\n <mtext>max</mtext>\n </msub>\n <mo>=</mo>\n </mrow>\n <annotation> ${r}_{\\text{max}}=$</annotation>\n </semantics></math> (79.5<span></span><math>\n <semantics>\n <mrow>\n <mo>±</mo>\n </mrow>\n <annotation> $\\pm $</annotation>\n </semantics></math>1.1) Jupiter radii for the Jovian magnetosphere, for the duration of the trajectory, suggesting a configuration with middling levels of expansion. We also predict the plasma conditions observed by Juno during the same flight-path, as well as the typical conditions over the orbit of Ganymede, with the magnetic and hot plasma pressures assuming dominant roles. Finally, these results are compared with functional fits of a compilation of Galileo flyby data obtained in the vicinity of Ganymede's orbit, suggesting Juno experienced somewhat similar conditions, despite a systematic overestimation in magnetic field intensity in the near-Ganymede space.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":null,"pages":null},"PeriodicalIF":2.6000,"publicationDate":"2024-10-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024JA032689","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA032689","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
We present an application of the latest UCL-AGA magnetodisc model (MDISC) to the study of the magnetic and plasma conditions in the near-Ganymede space. By doing this, we provide a comparison with measurements from Juno's most recent flyby of the Jovian moon, perijove 34 (PJ34). We find good agreement between the model results and the magnetometer data, pointing toward a hot plasma index value (2.7190.024)107 Pa m T−1 and an effective magnetodisc radius (79.51.1) Jupiter radii for the Jovian magnetosphere, for the duration of the trajectory, suggesting a configuration with middling levels of expansion. We also predict the plasma conditions observed by Juno during the same flight-path, as well as the typical conditions over the orbit of Ganymede, with the magnetic and hot plasma pressures assuming dominant roles. Finally, these results are compared with functional fits of a compilation of Galileo flyby data obtained in the vicinity of Ganymede's orbit, suggesting Juno experienced somewhat similar conditions, despite a systematic overestimation in magnetic field intensity in the near-Ganymede space.