“…Although the temperature rise due to the low energy dissipation of martensite reorientation in FSMA is negligible in the slow or quasi-static loading conditions, it cannot be ignored in high-frequency magnetic loadings (> 100 Hz) because the dissipation due to the frictional twin boundary motion of martensite reorientation (Blanter et al, 2007;Cui et al, 2017;He et al, 2012Heczko et al, 2016;Karaca et al, 2006;Lagoudas, 2005, 2004;Molnar et al, 2008;Murray et al, 2000;O'Handley et al, 2000;Pagounis et al, 2014;Yu et al, 2015) and the eddy current inside the material can accumulate quickly to induce significant temperature rise (Henry, 2002;Henry et al, 2002;Lai, 2009;Lai et al, 2008). Moreover, several physical properties related to martensite reorientation of FSMA are sensitive to the temperature (Aaltio et al, 2008;Adachi et al, 2017;Glavatska et al, 2002;Heczko et al, 2018;Heczko and Straka, 2003;Okamoto et al, 2008;Soroka et al, 2018;Sozinov et al, 2017;Straka et al, 2011aStraka et al, , 2006Straka et al, , 2016Straka et al, , 2012Vronka et al, 2017;Zreihan et al, 2016).…”