*PROTONEN ALS PRIMARE KOMPONENTE DER KOSMISCHEN STRAHLUNG .1.

[1] On the stopping of fast particles and on the creation of positive electrons [J]. PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-CONTAINING PAPERS OF A MATHEMATICAL AND PHYSICAL CHARACTER, 1934, 146 (A856) : 0083 - 0112

[2] Bethe H., 1933, HDB PHYS, V24, P273

[3] Stopping power of atoms with several electrons [J]. ZEITSCHRIFT FUR PHYSIK, 1933, 81 (5-6): : 363 - 376

[4] The influence of the earth's magnetic field on cosmic-ray intensities up to the top of the atmosphere [J]. PHYSICAL REVIEW, 1937, 52 (02): : 80 - 88

[5] BOWEN IS, 1938, PHYS REV, V53, P855

[6] Analysis of experiments on the scattering of protons by protons [J]. PHYSICAL REVIEW, 1939, 55 (11): : 1018 - 1064

[7] Burst production by mesotrons [J]. PHYSICAL REVIEW, 1941, 59 (05): : 414 - 421

[8] About the hard component of cosmic radiation in the stratosphere. [J]. ZEITSCHRIFT FUR PHYSIK, 1940, 115 (5-6): : 326 - 332

[9] EULER H, 1938, ERG EXAKT NATURWISS, V17, P1

[10] Heisenberg W., 1936, Z PHYS, V101, P533, DOI DOI 10.1007/BF01349603

[1] On the stopping of fast particles and on the creation of positive electrons [J]. PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-CONTAINING PAPERS OF A MATHEMATICAL AND PHYSICAL CHARACTER, 1934, 146 (A856) : 0083 - 0112

[2] Bethe H., 1933, HDB PHYS, V24, P273

[3] Stopping power of atoms with several electrons [J]. ZEITSCHRIFT FUR PHYSIK, 1933, 81 (5-6): : 363 - 376

[4] The influence of the earth's magnetic field on cosmic-ray intensities up to the top of the atmosphere [J]. PHYSICAL REVIEW, 1937, 52 (02): : 80 - 88

[5] BOWEN IS, 1938, PHYS REV, V53, P855

[6] Analysis of experiments on the scattering of protons by protons [J]. PHYSICAL REVIEW, 1939, 55 (11): : 1018 - 1064

[7] Burst production by mesotrons [J]. PHYSICAL REVIEW, 1941, 59 (05): : 414 - 421

[8] About the hard component of cosmic radiation in the stratosphere. [J]. ZEITSCHRIFT FUR PHYSIK, 1940, 115 (5-6): : 326 - 332

[9] EULER H, 1938, ERG EXAKT NATURWISS, V17, P1

[10] Heisenberg W., 1936, Z PHYS, V101, P533, DOI DOI 10.1007/BF01349603