Context. Aims. We systematically search for magnetic flux rope structures in the solar wind to within the closest distance to the Sun of ~0.13 AU, using data from the third and fourth orbits of the Parker Solar Probe. Methods. We extended our previous magnetic helicity-based technique of identifying magnetic flux rope structures. The method was improved upon to incorporate the azimuthal flow, which becomes larger as the spacecraft approaches the Sun. Results. A total of 21 and 34 magnetic flux ropes are identified during the third (21-day period) and fourth (17-day period) orbits of the Parker Solar Probe, respectively. Wemore »
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Zhao, L.-L. ; Zank, G. P. ; Adhikari, L. ; Hu, Q. ; Kasper, J. C. ; Bale, S. D. ; Korreck, K. E. ; Case, A. W. ; Stevens, M. ; Bonnell, J. W. ; et al ( , The Astrophysical Journal Supplement Series)
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O'Shea, E. ; Sternovsky, Z. ; Malaspina, D. M. ( , Journal of Geophysical Research: Space Physics)
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Kim, T. K. ; Pogorelov, N. V. ; Arge, C. N. ; Henney, C. J. ; Jones-Mecholsky, S. I. ; Smith, W. P. ; Bale, S. D. ; Bonnell, J. W. ; Dudok de Wit, T. ; Goetz, K. ; et al ( , The Astrophysical Journal Supplement Series)
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Bale, S. D. ; Badman, S. T. ; Bonnell, J. W. ; Bowen, T. A. ; Burgess, D. ; Case, A. W. ; Cattell, C. A. ; Chandran, B. D. ; Chaston, C. C. ; Chen, C. H. ; et al ( , Nature)
