Observations and modeling of the emerging EUV loops in the quiet Sun as seen with the Solar Dynamics Observatory

Autor: Chitta, LP., Kariyappa, R., van Ballegooijen, A. A., DeLuca, E. E., Hasan, S. S., Hanslmeier, A.

We used data from the Helioseismic and Magnetic Imager (HMI), and Atmospheric Imaging Assembly (AIA) on the \textit{Solar Dynamics Observatory} (SDO) to study coronal loops at small scales, emerging in the quiet Sun. With HMI line-of-sight magnetogra

Externí odkaz: http://arxiv.org/abs/1303.3426

Polarisation of decayless kink oscillations of solar coronal loops.

Autor: Zhong S; Centre for Fusion, Space and Astrophysics, Physics Department, University of Warwick, Coventry, CV4 7AL, UK., Nakariakov VM; Centre for Fusion, Space and Astrophysics, Physics Department, University of Warwick, Coventry, CV4 7AL, UK. V.Nakariakov@warwick.ac.uk.; Centro de Investigacion en Astronomía, Universidad Bernardo O'Higgins, Avenida Viel 1497, Santiago, Chile. V.Nakariakov@warwick.ac.uk., Kolotkov DY; Centre for Fusion, Space and Astrophysics, Physics Department, University of Warwick, Coventry, CV4 7AL, UK.; Engineering Research Institute 'Ventspils International Radio Astronomy Centre (VIRAC)' of Ventspils University of Applied Sciences, Inzenieru iela 101, Ventspils, LV-3601, Latvia., Chitta LP; Max Planck Institute for Solar System Research, D-37077, Göttingen, Germany., Antolin P; Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle Upon Tyne, NE1 8ST, UK., Verbeeck C; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, Brussels, 1180, Belgium., Berghmans D; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, Brussels, 1180, Belgium.

Publikováno v: Nature communications [Nat Commun] 2023 Sep 12; Vol. 14 (1), pp. 5298. Date of Electronic Publication: 2023 Sep 12.

Author Correction: Ultra-high-resolution observations of persistent null-point reconnection in the solar corona.

Autor: Cheng X; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China. xincheng@nju.edu.cn.; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany. xincheng@nju.edu.cn.; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China. xincheng@nju.edu.cn., Priest ER; School of Mathematics and Statistics, University of St. Andrews, Fife, KY16 9SS, Scotland, UK., Li HT; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China., Chen J; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China., Aulanier G; Sorbonne Université, Observatoire de Paris - PSL, École Polytechnique, IP Paris, CNRS, Laboratory for Plasma Physics (LPP), 4 place Jussieu, 75005, Paris, France.; Rosseland Centre for Solar Physics, Institute for Theoretical Astrophysics, Universitetet i Oslo, P.O. Box 1029, Blindern, 0315, Oslo, Norway., Chitta LP; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany., Wang YL; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China., Peter H; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany., Zhu XS; State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China., Xing C; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.; Sorbonne Université, Observatoire de Paris - PSL, École Polytechnique, IP Paris, CNRS, Laboratory for Plasma Physics (LPP), 4 place Jussieu, 75005, Paris, France., Ding MD; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China., Solanki SK; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany., Berghmans D; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, 1180, Brussels, Belgium., Teriaca L; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany., Aznar Cuadrado R; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany., Zhukov AN; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, 1180, Brussels, Belgium.; Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119992, Moscow, Russia., Guo Y; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China., Long D; Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK., Harra L; PMOD/WRC, Dorfstrasse 33, CH-7260, Davos Dorf, Switzerland.; ETH-Zürich, Wolfang-Pauli-Strasse 27, HIT J 22.4, 8093, Zürich, Switzerland., Smith PJ; Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK., Rodriguez L; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, 1180, Brussels, Belgium., Verbeeck C; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, 1180, Brussels, Belgium., Barczynski K; ETH-Zürich, Wolfang-Pauli-Strasse 27, HIT J 22.4, 8093, Zürich, Switzerland., Parenti S; Institut d'Astrophysique Spatiale, Université Paris-Saclay, 91405, Orsay Cedex, France.

Publikováno v: Nature communications [Nat Commun] 2023 Apr 25; Vol. 14 (1), pp. 2372. Date of Electronic Publication: 2023 Apr 25.

Defining the Middle Corona.

Autor: West MJ; Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 USA., Seaton DB; Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 USA., Wexler DB; Space Science Laboratory, University of Massachusetts Lowell, Lowell, Massachusetts USA., Raymond JC; Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA 02138 USA., Del Zanna G; DAMTP, CMS, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA UK., Rivera YJ; Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA 02138 USA., Kobelski AR; NASA Marshall Space Flight Center, Huntsville, AL 35812 USA., Chen B; New Jersey Institute of Technology, 323 Martin Luther King Jr. Blvd., Newark, NJ 07102 USA., DeForest C; Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 USA., Golub L; Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA 02138 USA., Caspi A; Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 USA., Gilly CR; Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 USA., Kooi JE; U.S. Naval Research Laboratory, Code 7213, 4555 Overlook Ave. SW, Washington, DC 20375 USA., Meyer KA; Mathematics, School of Science & Engineering, University of Dundee, Nethergate Dundee, DD1 4HN UK., Alterman BL; Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78238 USA., Alzate N; NASA Goddard Space Flight Center, Code 670, Greenbelt, MD 20771 USA.; ADNET Systems, Inc., Greenbelt, MD 20771 USA., Andretta V; INAF - Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy., Auchère F; Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, 91405 Orsay, France., Banerjee D; Indian Institute of Astrophysics, 2nd Block, Koramangala, Bangalore, 560034 India., Berghmans D; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan - 3 - Avenue Circulaire, 1180 Brussels, Belgium., Chamberlin P; Laboratory for Atmospheric and Space Physics, Space Science, 3665 Discovery Dr, Boulder, CO 80303 USA., Chitta LP; Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany., Downs C; Predictive Science Inc., 9990 Mesa Rim Rd, Suite 170, San Diego, CA 92121 USA., Giordano S; INAF-Astrophysical Observatory of Torino, via Osservatorio 20, I-10025 Pino Torinese, Italy., Harra L; ETH-Zürich, Hönggerberg campus, HIT building, Zürich, Switzerland., Higginson A; NASA Goddard Space Flight Center, Code 670, Greenbelt, MD 20771 USA., Howard RA; Applied Physics Laboratory, Johns Hopkins University, 11100 Johns Hopkins Rd., Laurel, MD 20723 USA., Kumar P; American University, Washington, DC 20016 USA.; NASA Goddard Space Flight Center, Code 670, Greenbelt, MD 20771 USA., Mason E; Predictive Science Inc., 9990 Mesa Rim Rd, Suite 170, San Diego, CA 92121 USA., Mason JP; Applied Physics Laboratory, Johns Hopkins University, 11100 Johns Hopkins Rd., Laurel, MD 20723 USA., Morton RJ; Department of Maths, Physics and Electrical Engineering, Northumbria University, Newcastle upon Tyne, UK., Nykyri K; Embry-Riddle Aeronautical University, 1 Aerospace Blvd., Daytona Beach, FL 32114 USA., Patel R; Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 USA., Rachmeler L; NOAA National Centers for Environmental Information, 325 Broadway, Boulder, CO 80305 USA., Reardon KP; National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303 USA., Reeves KK; Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA 02138 USA., Savage S; NASA Marshall Space Flight Center, Huntsville, AL 35812 USA., Thompson BJ; NASA Goddard Space Flight Center, Code 670, Greenbelt, MD 20771 USA., Van Kooten SJ; Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 USA., Viall NM; NASA Goddard Space Flight Center, Code 670, Greenbelt, MD 20771 USA., Vourlidas A; Applied Physics Laboratory, Johns Hopkins University, 11100 Johns Hopkins Rd., Laurel, MD 20723 USA., Zhukov AN; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan - 3 - Avenue Circulaire, 1180 Brussels, Belgium.; Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119992 Moscow, Russia.

Publikováno v: Solar physics [Sol Phys] 2023; Vol. 298 (6), pp. 78. Date of Electronic Publication: 2023 Jun 14.