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=====原子核乾板=====

===スキャン===

==参考文献==

  * 検出原理提案: K. Niwa et al., In Proc. Int. Cosmic Ray Symp. High Energy Phenomena, page 149 (1974).
  * Track Selector: S. Aoki et al., Nucl. Instrum. Methods Phys. Res. B, 51, 466-472 (1990).
  * New Track Selector: T. Nakano, Ph.D. thesis, Nagoya University (1997).
  * Ultra Track Selector: 
  * Super-Ultra Track Selector: K. Morishima and T. Nakano, JINST, 5, P04011 (2010).
  * NETSCAN: K. Hamada et al. JINST 7, P07001 (2012).
  * S-UTS & NETSCAN: K. Morishima et al., J. Rad. Meas., 50, 237-240 (2013).
  * Fine Track Selector: T. Fukuda et al., JINST, 8, P01023 (2013).
  * FTS for hadron: H. Ishida et al., Prog. Theor. Exp. Phys., 2014(9), 093C01 (2014).
  * FTS for MIP: T. Fukuda et al., JINST, 9, P12017 (2014).
  * Hyper Track Selector: M. Yoshimoto, et al., Prog. Theor. Exp. Phys., 2017(10), 103H01 (2017).
  * HTS & Large angle: Y. Suzuki et al., Prog. Theor. Exp. Phys., 2022(),  (2022).

===ランキングカット===

==参考文献==

  * OPERA CS: T. Fukuda et al., JINST, 5, P04009 (2010).
  * NINJA: Y. Suzuki et al., Prog. Theor. Exp. Phys., 2022(),  (2022).

===Volume Pulse Height===

==参考文献==

  * T. Toshito et al., Nucl. Instrum. Methods Phys. Res. A, 556, 482 (2006).

====GRAINE====

  * GRAINE で用いられた原子核乾板について
  * K. Ozaki et al., J. Instrum. 10, P12018 (2015).
  * AgBr 密度が高い乳剤 (55%) を用いることで OPERA フィルムにくらべて MIP の検出効率を 87% から97% に向上している．
  * OPERA のフィルムは機械で塗布するために乳剤の AgBr 密度に制限があった
  * Grain Density は ~50 / 100 um

  * Photon の偏極に対する感度について
  * K. Ozaki et al., Nucl. Instrum. Methods Phys. Res. A 833, 165--168 (2016).
  * 偏極によって生じる azimuthal angle 分布を高い角度分解能を用いて測定する
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