Early history of cosmic particle physics
Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not ju...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Walter, M. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2012 |
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| Schlagwörter: |
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| Anmerkung: |
© EDP Sciences and Springer 2012 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal - Berlin : Springer, 2010, 37(2012), 3 vom: 29. Juni, Seite 323-358 |
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| Übergeordnetes Werk: |
volume:37 ; year:2012 ; number:3 ; day:29 ; month:06 ; pages:323-358 |
| Links: |
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| DOI / URN: |
10.1140/epjh/e2012-30020-1 |
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| Katalog-ID: |
SPR030370345 |
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| 520 | |a Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. | ||
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10.1140/epjh/e2012-30020-1 doi (DE-627)SPR030370345 (SPR)e2012-30020-1-e DE-627 ger DE-627 rakwb eng Walter, M. verfasserin aut Early history of cosmic particle physics 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © EDP Sciences and Springer 2012 Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. Ionisation Chamber (dpeaa)DE-He213 Early History (dpeaa)DE-He213 Cosmic Radiation (dpeaa)DE-He213 Radioactive Substance (dpeaa)DE-He213 Soft Component (dpeaa)DE-He213 Wolfendale, A. W. aut Enthalten in The European physical journal Berlin : Springer, 2010 37(2012), 3 vom: 29. Juni, Seite 323-358 (DE-627)626052343 (DE-600)2553052-5 2102-6467 nnns volume:37 year:2012 number:3 day:29 month:06 pages:323-358 https://dx.doi.org/10.1140/epjh/e2012-30020-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4277 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 37 2012 3 29 06 323-358 |
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10.1140/epjh/e2012-30020-1 doi (DE-627)SPR030370345 (SPR)e2012-30020-1-e DE-627 ger DE-627 rakwb eng Walter, M. verfasserin aut Early history of cosmic particle physics 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © EDP Sciences and Springer 2012 Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. Ionisation Chamber (dpeaa)DE-He213 Early History (dpeaa)DE-He213 Cosmic Radiation (dpeaa)DE-He213 Radioactive Substance (dpeaa)DE-He213 Soft Component (dpeaa)DE-He213 Wolfendale, A. W. aut Enthalten in The European physical journal Berlin : Springer, 2010 37(2012), 3 vom: 29. Juni, Seite 323-358 (DE-627)626052343 (DE-600)2553052-5 2102-6467 nnns volume:37 year:2012 number:3 day:29 month:06 pages:323-358 https://dx.doi.org/10.1140/epjh/e2012-30020-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4277 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 37 2012 3 29 06 323-358 |
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10.1140/epjh/e2012-30020-1 doi (DE-627)SPR030370345 (SPR)e2012-30020-1-e DE-627 ger DE-627 rakwb eng Walter, M. verfasserin aut Early history of cosmic particle physics 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © EDP Sciences and Springer 2012 Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. Ionisation Chamber (dpeaa)DE-He213 Early History (dpeaa)DE-He213 Cosmic Radiation (dpeaa)DE-He213 Radioactive Substance (dpeaa)DE-He213 Soft Component (dpeaa)DE-He213 Wolfendale, A. W. aut Enthalten in The European physical journal Berlin : Springer, 2010 37(2012), 3 vom: 29. Juni, Seite 323-358 (DE-627)626052343 (DE-600)2553052-5 2102-6467 nnns volume:37 year:2012 number:3 day:29 month:06 pages:323-358 https://dx.doi.org/10.1140/epjh/e2012-30020-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4277 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 37 2012 3 29 06 323-358 |
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10.1140/epjh/e2012-30020-1 doi (DE-627)SPR030370345 (SPR)e2012-30020-1-e DE-627 ger DE-627 rakwb eng Walter, M. verfasserin aut Early history of cosmic particle physics 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © EDP Sciences and Springer 2012 Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. Ionisation Chamber (dpeaa)DE-He213 Early History (dpeaa)DE-He213 Cosmic Radiation (dpeaa)DE-He213 Radioactive Substance (dpeaa)DE-He213 Soft Component (dpeaa)DE-He213 Wolfendale, A. W. aut Enthalten in The European physical journal Berlin : Springer, 2010 37(2012), 3 vom: 29. Juni, Seite 323-358 (DE-627)626052343 (DE-600)2553052-5 2102-6467 nnns volume:37 year:2012 number:3 day:29 month:06 pages:323-358 https://dx.doi.org/10.1140/epjh/e2012-30020-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4277 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 37 2012 3 29 06 323-358 |
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Walter, M. |
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Early history of cosmic particle physics Ionisation Chamber (dpeaa)DE-He213 Early History (dpeaa)DE-He213 Cosmic Radiation (dpeaa)DE-He213 Radioactive Substance (dpeaa)DE-He213 Soft Component (dpeaa)DE-He213 |
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early history of cosmic particle physics |
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Early history of cosmic particle physics |
| abstract |
Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. © EDP Sciences and Springer 2012 |
| abstractGer |
Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. © EDP Sciences and Springer 2012 |
| abstract_unstemmed |
Abstract The discovery of cosmic rays is a standard example of ‘one man’s noise is another man’s signal’. From the apparently minor leakages of electricity from well-insulated detectors came a subject of great importance for modern science: the detection of a so-called ‘radiation’ coming from not just beyond the Earth’s atmosphere but from deep cosmic space. Furthermore, a radiation of energy density rivalling that of starlight. Our goal is to examine the history of the subject from the period of ‘pre-discovery’ in the years from 1900 to 1912, through the discovery itself up to the 1940’s when particle physics was continued with accelerators. The crucial role of ‘new techniques’, principally the Wulf electrometer and the Wilson cloud chamber and their use in precission studies by Hess, Kolhörster, Anderson and Blackett are described. The arguments about the veracity of Hess’s claim for an extra-terrestrial origin are included, as well as the developments leading to the inspired discovery of the positron and the muon. The question of ‘origin’ is also examined, from the contention by Hess that the Sun was not responsible, to the idea – still held – that supernovae are involved. © EDP Sciences and Springer 2012 |
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Early history of cosmic particle physics |
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https://dx.doi.org/10.1140/epjh/e2012-30020-1 |
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Wolfendale, A. W. |
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10.1140/epjh/e2012-30020-1 |
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2024-07-03T15:46:02.936Z |
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|
| score |
7.401636 |