“…Besides the peak in when the field is aligned near parallel to the film surface, there is a smaller peak when it is aligned near perpendicular to this surface This feature has been observed in HTS films [8], [9] and in some low temperature superconducting (LTS) films of NbTa [10], [11]. In the LTS films, it has sometimes been attributed to columnar grain boundary inhomogeneities [10], [11]. These columnar grain boundaries are essentially extended 2-D defects and are thought to produce stronger pinning in a situation in which the flux lines are aligned parallel to the columnar defect; the perpendicular flux lattice density will relate to the macroscopic pinning strength In the case of the HTS, it has sometimes been attributed to pinning along the spiral defects.…”