distinctive r.f. radiation events. In five instances, however, no effect is observed to accompany major chromospheric eruptions. The results cannot be accounted for solely on the basis of the expected impact zones for charged particles originating at the sun. Efforts are in progress to determine w
Nuclear resonance fluorescence in As75
โ Scribed by Franz R. Metzger
- Publisher
- Elsevier Science
- Year
- 1956
- Tongue
- English
- Weight
- 70 KB
- Volume
- 262
- Category
- Article
- ISSN
- 0016-0032
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โฆ Synopsis
With gaseous sources of Se76 in the form of selenium oxide, resonance scattering from the 265 kev leve1 in As'~ has been observed.'
Preliminary measurements indicate an isotopie distribution of the resonance radiation and thus favor assignment of spin 1/2 to the 265 kev leve1 in As'~. Self-absorption experiments indicate a mean life of 10~l1 second for the 265 kev transition. Although this lifetime is one order of magnitude longer than the prediction of the single particle model,2 it is considerably shorter than most Ml lifetimes.3 * Assisted by the joint program of the ONR and AEC. l For the disintegration scheme of S+, see, for example, A. W.
๐ SIMILAR VOLUMES
Using a source of As v4 in the form of arsine gas, a resonance fluorescence effect from the 635 kev level in Se v4 has been observed. Due to the small abundance of Se v4 (0.87 per cent), the effect is not very pronounced and the mean life of 6 X 10 -12 second, calculated from the magnitude of the re