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The Effect of the Io Plasma Torus on Precise Orbit Determination and Gravity Recovery Application to Europa ClipperThe neutral gases released by the intense volcanic activity of the Jupiter moon Io, once ionized by the Jupiter magnetic environment, give rise to a toroidal plasma distribution known as Io Plasma Torus (IPT). Radio signals passing through charged particles environments, such as the IPT, are heavily perturbed, proportionally to the rate of change of the charged particle distribution along the path of the radio wave. If not properly calibrated, the IPT may induce significant perturbation on the radiometric tracking link to Earth. The radio tracking signal is the main observable for the Gravity and Radio Science (G/RS) investigation on NASA’s Europa Clipper whose aim is to measure the gravity field, tidal response and moment of inertia of Europa, and to precisely reconstruct the trajectory of the probe in support to other scientific investigations. In this work we quantify the detrimental effect of the IPT on the radiometric observables. We show how this affects the products of the G/RS and prove the necessity for accurate calibrations. We simulate different calibration strategies to mitigate its perturbative effect, based on currently available models of the IPT. Considering that these models have been developed with Juno in mind, they are tailored to its orbital geometry and we show that they cannot be easily applied to other geometries. We conclude that although the model-based calibration strategies can be very effective, further work will be needed to make them applicable to probes with a significantly different orbital geometry, such as Europa Clipper or ESA’s JUICE.
Document ID
20250004922
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Gael Cascioli
(University of Maryland Baltimore Washington Medical Center Glen Burnie, Maryland, United States)
Erwan Mazarico
(Goddard Space Flight Center Greenbelt, United States)
Flavio Petricca
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Andrea Magnanini
(University of Bologna Bologna, Italy)
Dustin R Buccino
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Martina Ciambellini
(Sapienza University of Rome Rome, Lazio, Italy)
Antonio Genova
(Sapienza University of Rome Rome, Lazio, Italy)
Luis Gomez Casajus
(University of Bologna Bologna, Italy)
Marco Zannoni
(University of Bologna Bologna, Italy)
Paolo Tortora
(University of Bologna Bologna, Italy)
Date Acquired
May 12, 2025
Publication Date
March 30, 2025
Publication Information
Publication: The Planetary Science Journal
Publisher: IOP Publishing Ltd.
Volume: 6
Issue: 5
Issue Publication Date: May 30, 2025
e-ISSN: 2632-3338
Subject Category
Lunar and Planetary Science and Exploration
Funding Number(s)
OTHER: 2021-13- HH.1-2023
WBS: 684499.04.02.04
CONTRACT_GRANT: 80GSFC24M0006
CONTRACT_GRANT: 80NM0018D000
CONTRACT_GRANT: J-090027
CONTRACT_GRANT: J-090022
CONTRACT_GRANT: 80NM0018D0004
CONTRACT_GRANT: NNN12AA01C
CONTRACT_GRANT: J-090023
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
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