A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Jovian Electrons in the Inner Heliosphere : Opportunities for Multi-spacecraft Observations and Modeling
Tekijät: Strauss R. D., Dresing N., Engelbrecht N. E., Mitchell J. G., Kühl P., Jensen S., Fleth S., Sánchez-Cano B., Posner A., Rankin J. S, Lee C. O., van den Berg J. P., Ferreira S. E. S., Heber B.
Kustantaja: The American Astronomical Society
Julkaisuvuosi: 2024
Journal: Astrophysical Journal
Tietokannassa oleva lehden nimi: The Astrophysical Journal
Artikkelin numero: 57
Vuosikerta: 961
Numero: 1
DOI: https://doi.org/10.3847/1538-4357/ad11db
Verkko-osoite: https://dx.doi.org/10.3847/1538-4357/ad11db
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/386858819
Preprintin osoite: https://arxiv.org/abs/2401.02969
In this paper we explore the idea of using multi-spacecraft observations of Jovian electrons to measure the 3D distribution of these particles in the inner heliosphere. We present simulations of Jovian electron intensities along selected spacecraft trajectories for 2021 and compare these, admittedly qualitatively, to these measurements. Using the data–model comparison we emphasize how such a study can be used to constrain the transport parameters in the inner heliosphere, and how this can lead to additional insight into energetic particle transport. Model results are also shown along the expected trajectories of selected spacecraft, including the off-ecliptic phase of the Solar Orbiter mission from 2025 onward. Lastly, we revisit the use of historical data and discuss upcoming missions that may contribute to Jovian electron measurements.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
