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Particle Acceleration in Solar Flares and the Plasma Universe -- Deciphering its features under magnetic reconnection

15–19 Nov 2021
Virtual
US/Eastern timezone

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Session

Day 3 / Session 1

3-1
17 Nov 2021, 08:00
Virtual

Virtual

Conveners

Day 3 / Session 1

  • Tomoko Kawate

Presentation materials

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  1. 15. HXI onboard ASO-S
    Weiqun Gan (Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing. China)
    17/11/2021, 08:00
    Invited talk

    Advanced Space-based Solar Observatory (ASO-S) was officially approved in the end of 2017. The primary scientific objectives are to study the relationships between solar magnetic field, solar flares and coronal mass ejections. The are three payloads on it. By now the mission is in the stage of flight model and is planed to be launched in 2022. This talk will describe the general progress of...

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  2. 59. Numerical approaches for the understanding of particle acceleration during magnetic reconnection
    Shinsuke Takasao (Osaka University)
    17/11/2021, 08:30
    Invited talk

    TBD

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  3. 12. Magnetic reconnection as a key phenomenon in clusters of galaxies
    Kazuo Makishima (Kavli IPMU, The University of Tokyo)
    17/11/2021, 09:00
    Contributed talk

    The Intra-Cluster Medium (ICM), i.e., the ideal classical plasmas associated with individual cluster of galaxies (CLGs), is the most dominant known form of cosmic baryons. Within the ICM, the member galaxies move at transonic velocities, and their motion was long believed to be unaffected by the ICM. However, through a series of X-ray observations (from Makishima et al. 2001 to the latest one,...

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  4. 20. Constraints on the acceleration region of type III radio bursts from radio bursts and X-ray bursts
    Sophie Musset (ESA/ESTEC)
    17/11/2021, 09:15
    Contributed talk

    During the gradual phase of flare SOL2017-09-09T10:50, a faint increase of non-thermal X-ray emission has been detected by Fermi/GBM, and is associated with radio decimetric spikes and type III radio bursts detected by the ORFEES radio-spectrograph, the LOFAR radio-telescope, and the Wind/WAVE instrument. These signatures indicate that a faint acceleration event was the source of electron...

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