Cosmic‐ray‐produced electrons and gamma rays in the atmosphere

Reviews of Geophysics

Volumn 12, Issue 2, 1974, Pages 233-258

  Daniel, R R ^a   Stephens, S A ^a  

^a NONE

Author keywords

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Indexed keywords

EID: 84995084396     PISSN: 87551209     EISSN: 19449208     Source Type: Journal    
DOI: 10.1029/RG012i002p00233     Document Type: Review

References (113)

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2. Energy spectrum of individual gamma rays at balloon altitude
3. Production of lowenergy electrons
4. The detection and the measurement of energy of electron cascades in a small lead plate spark chamber
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6. Das Spectrum der Muonen, der Protonen und der Electronen in 5200 m Höhe
7. Energy dependence of the proton‐proton total crosssection for centre‐of‐mass energies between 23 and 53 GeV
8. Measurement of total proton‐proton cross‐section at ISR
9. The low energy gamma ray spectrum in space
10. Atmospheric gamma fays in the energy region 40‐1000 GeV
11. Cosmic ray electrons near sea level and at mountain altitudes
12. Etude de la composante molle du rayonnement cosmique au Pic du Midi
13. A study of the low energy electron component of the cosmic radiation
14. ‐2 atmospheric depth at Ft. Churchill
15. Negative particle production at the CERN intersecting storage rings
16. Secondary electrons and photons in the upper atmosphere
17. Secondary spectra of electrons and photons in the atmosphere
18. Cosmic ray negatron and positron spectra between 12 and 220 MeV
19. Cosmic ray negatron and positron spectra observed near Fort Churchill in 1968
20. On the penetrating component of cosmic radiation
21. Passage of fast electrons and the theory of cosmic showers
22. A balloon observation of high energy electrons
23. On multiplicative showers
24. Production of gamma rays in the atmosphere
25. Energy spectra of cosmic ray photons and electrons from plastic scintillation counter measurements
26. Scintillation counter study of energy spectra of cosmic ray photons and electrons at 11,200 ft.
27. Low energy gamma radiation in the atmosphere during active and quiet periods of the sun
28. Search for high energy cosmic gamma rays
29. Search for low‐energy interplanetary positrons
30. Interplanetary positrons near 1 MeV from other than the π → μ → e process
31. Cosmic ray electrons and positrons of energies 2 to 9.5 MeV observed in interplanetary space
32. Detection of interplanetary 3‐12 MeV electrons
33. Atmospheric gamma rays at balloon altitudes
34. Electron spectrum at 3200 m above sea level
35. Cosmic electrons and related astrophysics
36. Propagation of secondary electronphoton component of the cosmic radiation in the atmosphere in the region 1 MeV to 10 GeV
37. The diffuse cosmic gamma rays observed at an equatorial balloon altitude
38. Integral fluxes of primary cosmic rays at Palestine, Texas, and Fort Churchill, Canada, near solar minimum
39. Ratio of electrons to positrons in the primary cosmic radiation
40. The study of high energy gamma rays produced by cosmic radiation at 40,000 ft
41. The flux of gamma rays at high altitudes and comparison with the muon flux at sea‐level
42. Balloon measurements of the energy spectrum of cosmic electrons between 1 and 25 GeV
43. A magnetic core digitised spark chamber for space science experiment
44. The primary cosmic‐ray electron spectrum from 10 to 40 MeV
45. Charge composition and energy spectrum of primary cosmic ray electrons
46. Results of gamma ray balloon astronomy
47. Spark chamber for gamma ray astronomy
48. Search for solar and cosmic gamma rays
49. The energy dependence of positron‐electron ratio in the primary cosmic radiation in 1965
50. Production spectrum of gamma rays in high energy interaction, and high energy gamma ray intensity at 2990m
51. Videcon spark chamber system detector for gamma ray astronomy
52. The geomagnetic cut‐off at Ft. Churchill and the primary cosmic ray electron spectrum from 10 MeV to 12 GeV in 1968
53. The energy spectrum of primary cosmic ray electrons from 20 MeV to 20 GeV in 1968 and 1969
54. Cosmic ray electrons between 12 MeV and 1 GeV in 1961
55. Absolute calculations of secondary cosmic gamma rays at the top of the atmosphere
56. Diurnal intensity variation of low‐energy electrons observed near the polar cap
57. Cosmic‐ray‐produced low‐energy gamma rays
58. On the high energy soft component near sea level
59. On the high energy soft components at 2770m altitude
60. Low energy atmospheric gamma rays near geomagnetic equator
61. A study of high‐energy gamma rays at the top of the atmosphere
62. A study of high‐energy gamma rays at the top of the atmosphere
63. Search for primary cosmic gamma rays with satellite Explorer XI
64. A comparison of solar modulation effects on protons, electrons and helium nuclei
65. The primary cosmic ray electron spectrum near solar minimum
66. Flux and energy spectrum of primary cosmic ray electrons
67. A cloud chamber analysis of cosmic radiation at 3500 m, B, Results on the hard and soft components
68. A study of the production of α‐rays in high energy nuclear collisions
69. High energy electrons recorded on the ESRO‐II satellite
70. A search for energetic gamma ray emission from the supernova remnant Cassiopeia A
71. Cosmic rays in the galaxy
72. Flux and energy spectrum of cosmic ray electrons between 10 and 1000 GeV
73. Observation of the diffuse cosmic gamma radiation in the 30‐50 MeV region
74. The 0.511 MeV gamma ray measured with a Ge(Li) detector at the balloon altitude
75. Theory of cascade showers
76. The observation of electron component in the cosmic ray with emulsion chamber
77. Cosmic rays in the upper atmosphere
78. Flux and energy spectrum of secondary electrons in the upper atmosphere
79. The 0.5‐MeV gamma ray and the low‐energy gamma ray spectrum to 6 grams per square centimeter over Minneapolis
80. Gamma ray astronomy in space in the 50 KeV to 3 MeV region
81. A simple circuit for a phoswich scintillator counter
82. Low energy gamma ray measurements over Hyderabad, India
83. Galactic cosmic ray electrons
84. Gamma ray generation in the high atmosphere
85. A measurement of the spectrum of cosmic ray electrons between 20 MeV and 3 GeV in 1968—Further evidence for extensive time variations of this component
86. Primary cosmic ray electron spectrum between 5 and 300 GeV in 1968
87. Cosmic ray electron spectrum and its modulation near solar maximum
88. A study of vertical cutoff rigidities using sixth‐degree simulations of geomagnetic field
89. The primary cosmic ray electron spectrum from 10 GeV to about 200 GeV
90. Observation of cosmic ray electrons between 2.7 and 21.5 MeV
91. Cosmic ray electron flux above 4.7 GV
92. Superconducting magnetic spectrometer and cosmic ray nuclei
93. Atmospheric gamma rays of 1‐200 GeV over Hyderabad
94. Atmospheric electron spectrum over Hyderabad and a study of reentrant albedo electrons
95. 12eV) hadron collisions
96. Energetic gamma ray emission from the general direction of the Cygnus constellation
97. Evidence for change in the characteristics of strong interactions at ultra high energies
98. Measurement of the charged splash and reentrant albedo of the cosmic radiation
99. A calculation of the flux and energy spectrum of secondary electrons at high altitude in the atmosphere
100. A charged particle telescope for use in the measurements of the cosmic ray electron spectrum in the energy range 10 MeV‐2 BeV
101. A determination of the energy spectrum of extraterrestrial electrons in the energy range 70‐2000 MeV
102. Identifizierung von Protonen, Muonen und Elektronen in der weichen Komponente der Ultrastrahlung und Messung ihrer Energiespectren
103. High‐resolution search for solar gamma ray lines
104. Meson production at high energies and the propagation of cosmic rays through the atmosphere
105. Neutrino production in the atmosphere
106. The electron energy spectrum in the galactic cosmic ray flux in the region 5‐600 GeV