Giant Chromospheric Anemone Jet Observed with Hinode and Comparison with Magnetohydrodynamic Simulations: Evidence of Propagating Alfvén Waves and Magnetic Reconnection

By N. Nishizuka, M. Shimizu, T. Nakamura, Ken Otsuji, T. Okamoto, Y. Katsukawa, Kazunari Shibata. 2008

166 citations recorded by the source corpus.

Hinode discovered a beautiful giant jet with both cool and hot components at the solar limb on 2007 February 9. Simultaneous observations by the Hinode SOT, XRT, and TRACE 195 Å satellites revealed that hot (~5 × 106 K) and cool (~104 K) jets were located side by side and that the hot jet preceded the associated cool jet (~1-2 minutes). A current-sheet-like structure was seen in optical (Ca II H), EUV (195 Å), and soft X-ray emissions, suggesting that magnetic reconnection is occurring in the transition region or upper chromosphere. Alfvén waves were also observed with Hinode SOT. These propagated along the jet at velocities of ~200 km s−1 with amplitudes (transverse velocity) of ~5-15 km s−1 and a period of ~200 s. We performed two-dimensional MHD simulation of the jets on the basis of the emerging flux-reconnection model, by extending Yokoyama and Shibata’s model. We extended the model with a more realistic initial condition (~106 K corona) and compared our model with multiwavelength observations. The improvement of the coronal temperature and density in the simulation model allowed for the first time the reproduction of the structure and evolution of both the cool and hot jets quantitatively, supporting the magnetic reconnection model. The generation and the propagation of Alfvén waves are also reproduced self-consistently in the simulation model.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/375e89e323260f58673fc30043a41f2074fb29ff

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In Astronomy and Astrophysics

Citations in the corpus

The FIP and Inverse FIP Effects in Solar and Stellar Coronae (2015, background): “Observational evidence of low-lying reconnection producing jets and transverse waves of similar frequencies and amplitudes has been reported (Nishizuka et al., 2008; He et al., 2009; Vasheghani Farahani et al., 2009).”
THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS (2010, background): “…2007); chromospheric Hα surges (e.g., Schmahl 1981; Schmieder et al. 1995; Canfield et al. 1996; Chen et al. 2008); chromospheric Ca ii H jets (e.g., Nishizuka et al. 2008; Morita et al. 2010); coronal EUV microjets (Gurman et al. 1998); coronal X-ray jets (e.g., Shibata et al. 1992; Savcheva et…”