Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956

The experiments herein described are a continuation of similar experiments performed in previous years near the north geomagnetic pole. In 1954 low-energy particles were found at high altitudes which had the characteristics of protons with energies down to 150 Mev. In 1955 flights to higher altitude...

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Published in:Physical Review
Main Author: Neher, H. V.
Format: Article in Journal/Newspaper
Language:unknown
Published: Physical Review 1957
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Online Access:https://doi.org/10.1103/PhysRev.107.588
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spelling ftcaltechauth:oai:authors.library.caltech.edu:rre2w-dsr55 2024-06-23T07:52:58+00:00 Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956 Neher, H. V. 1957-07-15 https://doi.org/10.1103/PhysRev.107.588 unknown Physical Review https://doi.org/10.1103/PhysRev.107.588 oai:authors.library.caltech.edu:rre2w-dsr55 eprintid:8962 resolverid:CaltechAUTHORS:NEHpr57 info:eu-repo/semantics/openAccess Other Physical Review, 107(2), 588-592, (1957-07-15) info:eu-repo/semantics/article 1957 ftcaltechauth https://doi.org/10.1103/PhysRev.107.588 2024-06-12T03:13:34Z The experiments herein described are a continuation of similar experiments performed in previous years near the north geomagnetic pole. In 1954 low-energy particles were found at high altitudes which had the characteristics of protons with energies down to 150 Mev. In 1955 flights to higher altitudes (4 g cm^-2) indicated that these energies extended down to at least 100 Mev for protons. The numbers of both the high-energy particles (E>1 Bev) and those of low energy, in 1955 were less than in 1954. On one flight in 1955 the very low-energy particles were missing. In 1956, these low-energy particles (<300 Mev for protons) were missing completely. The "shape" of the ionization-depth curves at high altitudes appears to be a sensitive index of the presence or absence of these low-energy particles. In 1956 the "shape" of the curves at low pressures (<100 g cm^-2) was similar to those of 1951 when the low-energy radiation was missing and when a "knee" was present in the latitude curve at high altitudes. We infer that a "knee" was also present in 1956 but not in 1955. The fluctuations were also large in 1955 and 1956 compared with 1954. The average intensity of cosmic rays since 1954 has been decreasing with time as the sun approaches its maximum activity. This is in accordance with Forbush's relationship. However, in 1956 three of six flights showed intensities in the lower part of the atmosphere even less than any of the flights of 1937 at Saskatoon, Canada, in spite of the fact that the sun's activity in 1956 was less than in 1937. ©1957 The American Physical Society. Received 27 March 1957. The author wishes to take this opportunity to express his appreciation to the Office of Naval Research for making the arrangements necessary to carry out these experiments. He extends his thanks to the North East Air Command and the personnel at Thule Air Force Base for their help in making the flights and supplying the necessary helium. Finally, he wishes to thank Dr. Alan R. Johnston who helped with the ... Article in Journal/Newspaper Geomagnetic Pole Thule Air Caltech Authors (California Institute of Technology) Canada Physical Review 107 2 588 592
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collection Caltech Authors (California Institute of Technology)
op_collection_id ftcaltechauth
language unknown
description The experiments herein described are a continuation of similar experiments performed in previous years near the north geomagnetic pole. In 1954 low-energy particles were found at high altitudes which had the characteristics of protons with energies down to 150 Mev. In 1955 flights to higher altitudes (4 g cm^-2) indicated that these energies extended down to at least 100 Mev for protons. The numbers of both the high-energy particles (E>1 Bev) and those of low energy, in 1955 were less than in 1954. On one flight in 1955 the very low-energy particles were missing. In 1956, these low-energy particles (<300 Mev for protons) were missing completely. The "shape" of the ionization-depth curves at high altitudes appears to be a sensitive index of the presence or absence of these low-energy particles. In 1956 the "shape" of the curves at low pressures (<100 g cm^-2) was similar to those of 1951 when the low-energy radiation was missing and when a "knee" was present in the latitude curve at high altitudes. We infer that a "knee" was also present in 1956 but not in 1955. The fluctuations were also large in 1955 and 1956 compared with 1954. The average intensity of cosmic rays since 1954 has been decreasing with time as the sun approaches its maximum activity. This is in accordance with Forbush's relationship. However, in 1956 three of six flights showed intensities in the lower part of the atmosphere even less than any of the flights of 1937 at Saskatoon, Canada, in spite of the fact that the sun's activity in 1956 was less than in 1937. ©1957 The American Physical Society. Received 27 March 1957. The author wishes to take this opportunity to express his appreciation to the Office of Naval Research for making the arrangements necessary to carry out these experiments. He extends his thanks to the North East Air Command and the personnel at Thule Air Force Base for their help in making the flights and supplying the necessary helium. Finally, he wishes to thank Dr. Alan R. Johnston who helped with the ...
format Article in Journal/Newspaper
author Neher, H. V.
spellingShingle Neher, H. V.
Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956
author_facet Neher, H. V.
author_sort Neher, H. V.
title Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956
title_short Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956
title_full Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956
title_fullStr Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956
title_full_unstemmed Cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956
title_sort cosmic rays near the north geomagnetic pole in the summers of 1955 and 1956
publisher Physical Review
publishDate 1957
url https://doi.org/10.1103/PhysRev.107.588
geographic Canada
geographic_facet Canada
genre Geomagnetic Pole
Thule Air
genre_facet Geomagnetic Pole
Thule Air
op_source Physical Review, 107(2), 588-592, (1957-07-15)
op_relation https://doi.org/10.1103/PhysRev.107.588
oai:authors.library.caltech.edu:rre2w-dsr55
eprintid:8962
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op_rights info:eu-repo/semantics/openAccess
Other
op_doi https://doi.org/10.1103/PhysRev.107.588
container_title Physical Review
container_volume 107
container_issue 2
container_start_page 588
op_container_end_page 592
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