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Diagnostics of the Quiet Sun Atmosphere’s Photospheric Jets

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Abstract—From 2D-spectral observation data of a quiet region of the solar disk center in the Fe I λ 557.609 nm line, 3D hydrodynamic models of photospheric jets are built by solving the inverse radiative transfer problem. The obtained models describe thermodynamic parameters and the complete velocity field (vertical and horizontal). It is shown that the photospheric jets under consideration arise from the interaction of the surrounding environment with the field of the magnetic tube. The jets are located in a region of a unipolar magnetized downflow at the impact point of two horizontal flows, and they tend to occur at the edge of magnetic tubes. The observed gas velocities are subsonic in downflows of the jets. Energy release in the photospheric jets is predominantly localized in the middle photosphere layers, where the excess pressure is maximal. Compared with the surrounding media, mass density in the jets is significantly increased in the upper layers and slightly decreased in the lower layers of the photosphere.

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  1. Courtesy of N.G. Shchukina.

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ACKNOWLEDGMENTS

We are grateful to M.S.G. Löfdahl for providing technical observation data on SST/CRISP and for training on the use of the CRISPRED data-processing pipeline. The Swedish 1-m solar telescope operates on La Palma Island under the guidance of the Institute of Solar Physics at the University of Stockholm in the Spanish Observatory Roque de los Muchachos at the Canary Institute of Astrophysics. A.V. Sukhorukov is grateful to the Ministry of Economy and Business of Spain for financial support.

Funding

The work was carried out with the partial support of the Ministry of Education and Science of Ukraine at the Ivan Franko National University of Lviv in the framework of research work on the project AO-91F. The work was financially supported by the Ministry of Economy and Business of Spain in the framework of the 2015 Severo Ochoa program, registration number SEV-2015-0548.

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Authors and Affiliations

  1. Astronomical Observatory, Ivan Franko National University of Lviv, Lviv, Ukraine

    M. I. Stodilka

  2. Main Astronomical Observatory, National Academy of Sciences of Ukraine, Kyiv, Ukraine

    A. V. Sukhorukov & A. I. Prysiazhnyi

  3. Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain

    A. V. Sukhorukov

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Translated by S. Avodkova

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Stodilka, M.I., Sukhorukov, A.V. & Prysiazhnyi, A.I. Diagnostics of the Quiet Sun Atmosphere’s Photospheric Jets. Kinemat. Phys. Celest. Bodies 35, 231–251 (2019). https://doi.org/10.3103/S0884591319050040

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