Thc variation is given for ionisation, primaries and showers undcr layers of 56 to 78 ern of iron under the influence of barometric variations. Its value is 2% for I ern of Hg, which is much larger than could be expected from the decrease of hard primaries, which is proportional to density.
Decrease of primaries, showers and ionisation of cosmic rays under layers of lead and iron
β Scribed by J. Clay; A. van Gemert; J.T. Wiersma
- Publisher
- Elsevier Science
- Year
- 1936
- Weight
- 543 KB
- Volume
- 3
- Category
- Article
- ISSN
- 0031-8914
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β¦ Synopsis
The number of showers of Cosmic Rays was measured in lead cylinders under layers of iron and lead up to 700 gr/cm t β’ The number of showers under iron and lead sheets was also measured.
Under lead and iron were found two maxima which are explained by the two kinds of primaries both of which produce showers. From the place of the maximum and the coefficient of decrease of the hard primaries the coefficient for the decrease of the showers of the primaries was calculated and after that a calculation could be made for the decrease of the soft primaries and their showers. The curves based on these calculations showed a good agreement with the observations. The fact, that the first maximum in the shower curve isnot found under thick layers is here explained by the absence of the soft primaries in this case.
A comparison was made of the decrease of primaries and of showers with that of ionisation under layers of lead and iron between 400 and 700 gr/cm t β’ From this we see that the decrease is the same and previous results under water are confirmed. The decrease is 0.00042 per gr/cm t β’
π SIMILAR VOLUMES
Since the lower atmospheric layers give a much' larger decrease of primary rays than found for layers of lead, iron and water of the same mass per em' the possibility is considered that nitrogen might act abnormally on the rays. In consideration of this possibility the decrease in ureurn, CO(XH,l,
From the combination of Latitude effect and East--West asymmetry it is possible to conclude whether there are positive and negative primaries. Our observations give a ratio of the number of positives to negatives of about 2 to 1, between two given energy limits. A north excess of 4% is found in Ban