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Radial evolution of the accuracy of ballistic solar wind backmapping
DOI: 10.1051/0004-6361/202348892 Bibcode: 2024A&A...686A..12D

Maksimovic, M.; Démoulin, P.; Badman, S. T. +4 more

Context. Solar wind backmapping is a technique employed to connect in situ measurements of heliospheric plasma structures to their origin near the Sun. The most widely used method is ballistic mapping, which neglects the effects of solar wind acceleration and corotation and instead models the solar wind as a constant radial outflow whose speed is …

2024 Astronomy and Astrophysics
Ulysses 10
Evolution of coronal mass ejections with and without sheaths from the inner to the outer heliosphere: Statistical investigation for 1975 to 2022
DOI: 10.1051/0004-6361/202348641 Bibcode: 2024A&A...685A..89L

Temmer, M.; Larrodera, C.


Aims: This study covers a thorough statistical investigation of the evolution of interplanetary coronal mass ejections (ICMEs) with and without sheaths through a broad heliocentric distance and temporal range. The analysis treats the sheath and magnetic obstacle (MO) separately in order to gain more insight on their physical properties. In de…

2024 Astronomy and Astrophysics
Ulysses 4
The unexpected role of heliospheric boundaries in facilitating interstellar dust penetration at 1-5 AU
DOI: 10.1051/0004-6361/202450257 Bibcode: 2024A&A...687L...4G

Izmodenov, V. V.; Godenko, E. A.


Aims: Interstellar dust (ISD) particles penetrate the heliosphere because of the relative motion of the local interstellar cloud and the Sun. The penetrated particles pass through the heliospheric interface, that is, the region in which solar wind and interstellar plasma interact. As a result, the ISD flow is modified after the passage throug…

2024 Astronomy and Astrophysics
Ulysses 1