[en] Progress on nuclear reaction and nuclear structure studies is briefly reported. Reactions studied are (t,³He) reactions on various targets

[en] A review of the evidence on the properties of the nuclei with A = 5, 6, 7, 8, 9 and 10 nuclei, with emphasis on material leading to information about the structure of the A = 5-10 systems. (orig.)

[en] A selected list of reviews which contain useful nuclear data summaries or compilations is presented. (U.S.)

[en] Compilation of energy levels of A=11 and 12 nuclei, with emphasis on material leading to information about the structure of the A=11 and 12 systems. (orig.)

[en] Compilation of energy levels of A = 5, 6, 7, 8, 9 and 10 nuclei, with emphasis on material leading to information about the structure of the A = 5-10 systems. (Auth.)

[en] An attempt has been made to describe the spectroscopy of a few of the light nuclei and to point out some of the reasons why the light nuclei have been and are intensively studied. 10 refs.; 5 figs

[en] Reasons for the recent widespread interest in light nuclei are presented and some problems are discussed. States of a particular character, say 1⁺ states, or 4^- states, can be preferentially excited, and observed, using hitherto unavailable probes and techniques, and nuclei far off the valley of stability, such as ⁸He and ⁸C can now be routinely created. Beams of electrons, pions, kaons, antiprotons and heavy ions at high energies are all available with high resolution. The second reason is that the increased interest in and sophistication of astrophysical calculations require the measurement of many cross sections involved in nucleosynthesis. Thirdly, populations of states in the light nuclei have been used as signatures for what happens when heavy nuclei collide at high energies. The fourth reason is that many of the states in the light nuclei are so well understood that they can be used to test fundamental processes in the laboratory. Lastly, the light nuclei, whose states are well separated at low excitation energies, can be used to test nuclear reaction models. (author)

[en] Compilation of energy levels of A=13, 14 and 15 nuclei, with emphasis on material leading to information about the structure of the A=13, 14 and 15 systems. (orig.)

[en] Compilation of energy levels of A = 13, 14 and 15 nuclei, with emphasis on material leading to information about the structure of the A = 13, 14 and 15 systems. (orig.)

[en] Review of the information on several light isobars is given with concentration on experiments since 1984 and on reactions which generally do not involve heavy ions. The isobars with A=6,7,14,16,18,20 are considered