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Observation and modelling of solar jets
DOI: 10.1098/rspa.2020.0217 Bibcode: 2021RSPSA.47700217S

Shen, Yuandeng

The solar atmosphere is full of complicated transients manifesting the reconfiguration of the solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma ejections; they are ubiquitous in the solar atmosphere and important for our understanding of solar activities at different scales, the magnetic reconnection process, parti…

2021 Proceedings of the Royal Society of London Series A
IRIS 97
Three-dimensional magnetic reconnection in astrophysical plasmas
DOI: 10.1098/rspa.2020.0949 Bibcode: 2021RSPSA.47700949L

Li, Ting; Priest, Eric; Guo, Ruilong

Magnetic reconnection is a fundamental process in laboratory, magnetospheric, solar and astrophysical plasmas, whereby magnetic energy is converted into heat, bulk kinetic energy and fast particle energy. Its nature in two dimensions is much better understood than that in three dimensions, where its character is completely different and has many d…

2021 Proceedings of the Royal Society of London Series A
SOHO 34