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Workshop: Kinetic physics of astrophysical plasmas

18–20 mai 2026
Montpellier
Fuseau horaire Europe/Paris

Contact

Session

Magnetic Reconnection

20 mai 2026, 09:00
Bâtiment 20 Amphithéâtre (Montpellier)

Bâtiment 20 Amphithéâtre

Montpellier

Université de Montpellier – Campus Triolet

Description

Invited Speakers: N. Aunai (LULI), V. Brunn (Obs Arcetri, Italy), S. Masson (LPP)

Documents de présentation

Aucun document.

  1. 52. TBA
    Dr Pierre Henri ((1) Laboratoire Lagrange, Observatoire Côte d'Azur, Université Côte d'Azur, CNRS, Nice, France & (2) LPC2E, CNRS, Univ. Orléans, CNES, Orléans, France)
    20/05/2026 09:25
  2. 54. Contribution 5
    20/05/2026 10:25
  3. 55. Solar energetic particles : observations and modelling
    Dr Sophie Masson (LPP - Observatoire de Paris)
    20/05/2026 11:30

    Solar eruptions are initiated and develop in the solar corona and are one of the most extreme manifestation of the sun impulsive release of energy. Solar particles are accelerated during solar eruption. We observe their radiative signatures in the solar atmosphere over a large range of wavelengths from EUV to gamma rays and measure them in-situ in the heliosphere. Solar energetic particles...

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  4. 58. A new view on magnetic reconnection in the Earth’s magnetosphere
    Dr Nicolas Aunai
    20/05/2026 14:00

    Magnetic reconnection at Earth’s magnetopause is the key process controlling the coupling between the solar wind and the magnetosphere, enabling plasma and magnetic flux from the interplanetary medium to enter an otherwise largely closed cavity. A central question is where reconnection develops along the magnetopause, since its location strongly influences the efficiency of this coupling....

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  5. 53. Contribution 6
    M. Enzo Figueiredo
    20/05/2026 15:00
  6. 59. In-situ particle acceleration by magnetic reconnection in young stellar objects
    Dr Valentin Brunn (Arcetri Observatory)
    20/05/2026 15:50

    Young stellar objects host strongly magnetised and highly variable plasma environments in which several acceleration processes may generate suprathermal and non-thermal particles. In this talk, I will discuss two complementary regimes of particle acceleration in the star-disc system. The first is associated with large-scale magnetic reconnection during flares in the innermost regions, where...

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  7. 56. Contribution 11
  8. 57. Contribution 9
  9. 60. Discussion
Ordre du jour en construction...