  Jet phenomena with a bright loop in their footpoint, called anemone jets,
have been observed in the solar corona and chromosphere. These jets are formed
as a consequence of magnetic reconnection, and from the scale universality of
magnetohydrodynamics (MHD), it can be expected that anemone jets exist even in
the solar photosphere. However, it is not necessarily apparent that jets can be
generated as a result of magnetic reconnection in the photosphere, where the
magnetic energy is not dominant. Furthermore, MHD waves generated from the
photospheric jets could contribute to chromospheric heating and spicule
formation; however, this hypothesis has not yet been thoroughly investigated.
In this study, we perform 3D MHD simulation including gravity with the solar
photospheric parameter to investigate anemone jets in the solar photosphere. In
the simulation, jet-like structures were induced by magnetic reconnection in
the solar photosphere. We determined that these jet-like structures were caused
by slow shocks formed by the reconnection and were propagated approximately in
the direction of the background magnetic field. We also suggested that MHD
waves from the jet-like structures could influence local atmospheric heating
and spicule formation.
