“…In many cases the structure and internal stratigraphy of these masses are complex and difficult to determine, given the vagaries of exposure at any one time. However, over a hundred years of careful observation of the constantly changing patterns of exposure (Lyell, 1840;Trimmer, 1847;Reid, 1882;Bonney & Hill, 1905;Brydone, 1906Brydone, , 1908Brydone, , 1909Brydone, , 1938Peake & Hancock, 1961, 1970Wood, 1967Wood, , 1988 have produced a relatively clear understanding of the overall geometry and structure of most of the masses. Many of these masses are completely enclosed within the till.…”