Details

Autor(en) / Beteiligte

• Geiger, H.
• Rutherford, Lord
• Regener, E.
• Lindemann, F. A.
• Wilson, C. T. R.
• Chadwick, J.
• Gray, L. H.
• Tarrant, G. T. P.
• Dobson, G. M. B.
• Bragg, William
• Richardson, O. W.
• Eddington, Arthur
• Soddy, F.
• Chapman, S.

Titel

Discussion on ultra-penetrating rays

Ist Teil von

• Proceedings of the Royal Society of London. Series A, Containing papers of a mathematical and physical character, 1931-07, Vol.132 (819), p.331-352

Ort / Verlag

London: The Royal Society

Erscheinungsjahr

1931

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• About 20 years ago we first noted the presence of a γ-type-radiation of high penetrability probably of cosmic origin passing through the atmosphere. The first fundamental experiments carried out by Hess and improved on by Kolhörster, in which an air-tight electrometer registered the ionisation-current at different altitudes, showed us that the current increased with the altitude; at not more than a few thousand metres the current was several times larger than at sea-level. These results indicated the presence of an extremely penetrating radiation which seemed to be markedly absorbed by the atmosphere above us. Great difficulties were met with in studying the nature of this remarkable radiation due principally to its extremely weak intensity, high penetrability and lack of properties affected by external influences. Our knowledge progressed slowly and only after many years of experiment were we able to say that the penetrability is about ten times greater than the hard γ-rays of radium, and that the ionisation in air at sealevel is slightly more than 1 ion per second per cubic centimetre. We were able to add that in the explorable regions of the atmosphere the radiation was diffuse and, further, there seemed to be no relation to the daily movement of the sun. Even at the present time we cannot say with certainty that the variations observed in the intensity of the radiation are wholly of atmospheric origin or partly an intrinsic property. The doubtful origin and nature of this radiation continued to occupy our attention. The old experimental methods had been exhausted and new ones had to be evolved to insure a better understanding of the problem. In recent years we have progressed in two directions, namely, along electrometric lines by the improvement of the registration and the application of high pressure chambers, and by the method of electron counting. In the pressure chamber the degree of ionisation produced in the gas by the ultra-radiation is measured, while in the tube electron counter the high velocity electrons present with the ultra-radiation are singly registered.