A comparison of various procedures for fine grain development in electron microscopic radioautography

Abstract

Fine grain development for electron microscopic radioautography was investigated with two types of radioactive specimens: sections of tritiated methacrylate, which provide a homogeneously labeled source for quantitative evaluation of the radioautographic reaction, and sections of 125I-labeled thyroid. Radioautographs were prepared with Ilford L4, Sakura NR-H2, Agfa-Gevaert NUC 307 or Kodak NTE emulsions. The radioautographs were developed with one of several "solution physical" development procedures (Agfa-Gevaert, phenidone-ascorbic acid, p-phenylenediamine developers) or with arrested "direct" developments (D-19b, Elon-ascorbic acid developers). By arresting each development at an early stage of the reaction and at progressively longer time intervals, it was possible to examine the sequence of shapes in the growth of developed silver deposits for each emulsion-development combination. Thus, conditions which resulted in the development of small, round, compact silver deposits were defined for each emulsion. These developments were used in conjuction with gold latensification, a treatment which increases the sensitivity of the emulsions and thus compensates for the lowered sensitivity of fine grain development procedures. The location of the silver deposits in relation to the silver bromide crystals from which they derive was investigated. The emulsion gelatin surrounding the crystals was stained whereas the spaces, which remained after the crystals were dissolved in the photographic fixer, appeared transparent. This analysis permitted the selection of development procedures in which the single or multiple round silver deposits originating from a single crystal will remain within or on the boundary of this crystal. By this method, quantitation of radioautographic reactions composed of small, round silver deposits was studied by using the uniformly labeled 3H-methacrylate sections as a standard source of radiation. The conditions under which grain counting is feasible are discussed.