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the RMHD simulation. These properties are the manifestation of
the transition process from the ambient twisted field to the axial
field, which is consistent with the upwardly propagating non-linear
Alfve´ nic waves. The triggering process is still under investigation,
although we considered that the key mechanisms would the flux
merger, downflow along the core, or magnetic reconnection above
the twisted field.
Our prediction will be a useful tool for distinguishing the driving
mechanisms of chromospheric jets when combined with future
observations, such as SUNRISE III, DKIST, or EST. An appropriate
time cadence, integration time, and field of view should be selected
to fully capture the characteristic magnetic field associated with the
chromospheric jets.
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