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K. Barczynski on Muck Rack

K. Barczynski

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

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By X. Cheng, H. Li, G. Aulanier, L. P. Chitta, Y. L. Wang, H. Peter, M. D. Ding, S. K. Solanki, L. Teriaca, R. Cuadrado, A. N. Zhukov, Y. -W. Guo, D. Long, P. J. Smith, C. Verbeeck, K. Barczynski
| Nature Verified
Correction to: Nature Communications https://doi.org/10.1038/s41467-023-37888-w, published online 13 April 2023 In this article the grant number ERC, ORIGIN, 101039844, relating to funding by the European Union for L. P. Chitta was omitted. The original article has been corrected. Author information Authors and Affiliations School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China X. Cheng, H. T. Li, J. Chen, Y. L. Wang, C. Xing, M. D. Ding & Y.
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Ultra-high-resolution observations of persistent null-point reconnection in the solar corona - Nature Communications

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By X. Cheng, H. Li, L. P. Chitta, Y. L. Wang, H. Peter, M. D. Ding, S. K. Solanki, R. Cuadrado, A. N. Zhukov, Y. -W. Guo, D. Long, P. J. Smith, G. Aulanier, L. Teriaca, C. Verbeeck, K. Barczynski
| Nature Verified
Instruments and data We mainly used the EUI/HRIEUV 174 Å level 2 data (https://doi.org/10.24414/2qfw-tr95). The dataset are also part of SolO Observing Plan for studying the origin of slow solar wind. The field of view (FOV) of the EUI/HRIEUV is ~\({16.8}^{{\prime} }\times 16.{8}^{{\prime} }\) with a pixel size of 0.492″, which corresponds to a linear scale of about 195 km at this distance. The remaining spacecraft jitter was removed by a cross-correlation technique73.
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