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Astronomy and Space Physics

Joan Jordi Boldu O Farrill Treviño (Uppsala University/IRF): The Role of Kinetic Waves in the Solar Wind Evolution (Pre-defence seminar)

Europe/Stockholm
10132Å

10132Å

Description

Title: The Role of Kinetic Waves in the Solar Wind Evolution
Speaker: Joan Jordi Boldu O Farrill Treviño
Affiliation: Uppsala University/IRF
Time: Monday 3 November 2025, 15:15 to 16:15
Location: 10132Å, Häggsalen, Ångström

Abstract:  
Charged particles constantly stream outward from the Sun to fill the heliosphere. These particles, consisting mainly of protons and electrons, form a plasma called the solar wind. While the general structure of the solar wind was established decades ago, the radial evolution of its properties, such as temperature and velocity distributions, remains poorly understood.  Conventional fluid models fail to explain observed solar wind behavior because of its low collisionallity. Therefore, the radial evolution of the solar wind properties must be driven by collisionless processes. In particular  wave-particle interactions occuring at kinetic scales are an important regulator of the solar wind properties, because of the strong connection between the electromagnetic fields and the charged particles. We investigate the effect of kinetic waves in the solar wind evolution, demonstrating the necessity of a kinectic treatment to accurately describe the fundamental physics of the heliosphere.