Plasma and Fusion Research

Volume 18, 1402058 (2023)

Regular Articles


A Comparison of Velocimetry Algorithms: Orthogonal Dynamic Programming Based Particle Image Velocimetry Versus Local Correlation Tracking
Tatsuya KOBAYASHI1,2), Ryohtaroh T. ISHIKAWA3,4), Motoki NAKATA1,2), Takayoshi OBA3) and Yukio KATSUKAWA3)
1)
National Institute for Fusion Science, National Institutes of Natural Sciences, Toki 509-5292, Japan
2)
The Graduate University for Advanced Studies, SOKENDAI, Toki 509-5292, Japan
3)
National Astronomical Observatory of Japan, Mitaka 181-8588, Japan
4)
Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8603, Japan
(Received 1 May 2023 / Accepted 31 May 2023 / Published 14 July 2023)

Abstract

In the magnetic plasma fusion community and the solar physics research community, different velocimetry algorithms have been used. Those are: orthogonal dynamic programing based particle image velocimetry (ODP-PIV) and local correlation tracking (LCT), respectively. In this paper, a systematic comparison of these velocimetry codes is performed using synthetically produced turbulence data. The spatial scale of a typical turbulence pattern is scanned to examine the sensitivity of these codes on the tracer pattern property. Use of an LCT code is recommended when the ratio of the turbulence pattern size to the spatial resolution is small.


Keywords

plasma turbulence, magnetic fusion plasma, solar physics, velocimetry, orthogonal dynamic programming, local correlation tracking

DOI: 10.1585/pfr.18.1402058


References

  • [1] H. Biglari, P.H. Diamond and P.W. Terry, Phys. Fluids B 2, 1 (1990).
  • [2] T. Kobayashi, Nucl. Fusion 60, 095001 (2020).
  • [3] T. Ido, Y. Hamada, A. Nishizawa, Y. Kawasumi, Y. Miura and K. Kamiya, Rev. Sci. Instrum. 70, 955 (1999).
  • [4] R.J. Groebner, K.H. Burrell and R.P. Seraydarian, Phys. Rev. Lett. 64, 3015 (1990).
  • [5] K. Ida, S. Hidekuma, Y. Miura, T. Fujita, M. Mori, K. Hoshino, N. Suzuki, T. Yamauchi, JFT-2M group et al., Phys. Rev. Lett. 65, 1364 (1990).
  • [6] M. Yoshinuma, K. Ida, M. Yokoyama, M. Osakabe and K. Nagaoka, Fusion Sci. Technol. 58, 375 (2010).
  • [7] G.R. McKee, R.J. Fonck, D.K. Gupta, D.J. Schlossberg, M.W. Shafer, C. Holland and G. Tynan, Rev. Sci. Instrum. 75, 3490 (2004).
  • [8] T. Kobayashi, M. Yoshinuma and K. Ida, Plasma Phys. Control. Fusion 62, 125011 (2020).
  • [9] H. Park, E. Mazzucato, T. Munsat, C.W. Domier, M. Johnson, N.C. Luhmann Jr, J.Wang, Z. Xia, I.G.J. Classen, A.J.H Donné et al., Rev. Sci. Instrum. 75(10), 3787 (2004).
  • [10] G.M. Quénot, J. Pakleza and T.A. Kowalewski, Exp. Fluids 25, 177 (1998).
  • [11] D.K. Gupta, G.R. McKee and R.J. Fonck, Rev. Sci. Instrum. 81, 013501 (2010).
  • [12] Z. Yan, G.R. McKee, R. Fonck, P. Gohil, R.J. Groebner and T.H. Osborne, Phys. Rev. Lett. 112, 125002 (2014).
  • [13] A. Diallo, S. Banerjee, S.J. Zweben and T. Stoltzfus-Dueck, Nucl. Fusion 57, 066050 (2017).
  • [14] S. Banerjee, H. Zushi, N. Nishino, K. Mishra, T. Onchi, A. Kuzmin, Y. Nagashima, K. Hanada, K. Nakamura, H. Idei et al., Rev. Sci. Instrum. 86, 033505 (2015).
  • [15] S.J. Zweben, A. Diallo, M. Lampert, T. Stoltzfus-Dueck and S. Banerjee, Phys. Plasmas 28, 032304 (2021).
  • [16] T. Kobayashi, G. Birkenmeier, E. Wolfrum, F.M. Laggner, M. Willensdorfer, U. Stroth, S. Inagaki, S.-I. Itoh and K. Itoh, Rev. Sci. Instrum. 85, 083507 (2014).
  • [17] S. Toriumi and H. Wang, Living Rev. Sol. Phys. 16, 3 (2019).
  • [18] S.R. Cranmer and A.R. Winebarger, Annu. Rev. Astron. Astrophys. 57, 157 (2019).
  • [19] L.J. November and G.W. Simon, Astrophys. J. 333, 427 (1998).
  • [20] M. Rieutord and F. Rincon, Living Rev. Sol. Phys. 7, 1 (2010).
  • [21] T. Darvann, Master's thesis, University of Oslo, 1991.
  • [22] R. Molowny-Horas and Z. Yi, ITA (Oslo) Int. Rep. page 31 (1994).
  • [23] G.H. Fisher and B.T.Welsch, FLCT: a fast, efficient method for performing local correlation tracking, In Subsurface and atmospheric influences on solar activity, vol. 383, p.373 (2008).
  • [24] R.T. Ishikawa, M. Nakata, Y. Katsukawa, Y. Masada and T.L. Riethmüller, Astron. Astrophys. 658, A142 (2022).