Dwyer, R. (1978) The mean mass of the abundant cosmic-ray nuclei from boron to silicon at 1.2 GeV per atomic mass unit. The Astrophysical Journal, 224. 691pp. doi:10.1086/156417

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Reference Type	Journal (article/letter/editorial)
Title	The mean mass of the abundant cosmic-ray nuclei from boron to silicon at 1.2 GeV per atomic mass unit
Journal	The Astrophysical Journal
Authors	Dwyer, R.		Author
Year	1978 (September)	Volume	224
Publisher	IOP Publishing
DOI	doi:10.1086/156417Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	3312464	Long-form Identifier	mindat:1:5:3312464:9
GUID	0
Full Reference	Dwyer, R. (1978) The mean mass of the abundant cosmic-ray nuclei from boron to silicon at 1.2 GeV per atomic mass unit. The Astrophysical Journal, 224. 691pp. doi:10.1086/156417
Plain Text	Dwyer, R. (1978) The mean mass of the abundant cosmic-ray nuclei from boron to silicon at 1.2 GeV per atomic mass unit. The Astrophysical Journal, 224. 691pp. doi:10.1086/156417
In	(1978) The Astrophysical Journal Vol. 224. IOP Publishing

	*Dwyer, R., Meyer, P. (1977) Mean mass of cosmic-ray Ne, Mg, SI at 1.2 GeV/amu. The Astrophysical Journal, 216. 646pp. doi:10.1086/155504*
	*Dwyer, R., Meyer, P. (1985) Composition of cosmic-ray nuclei from boron to nickel for 1200 to 2400 MeV per nucleon. The Astrophysical Journal, 294. 441pp. doi:10.1086/163310*
	*Dwyer, Robert, Meyer, Peter (1987) Cosmic-ray elemental abundances from 1 to 10 GeV per AMU for boron through nickel. The Astrophysical Journal, 322. 981pp. doi:10.1086/165793*
	Woods, R. T., Hart, H. R., Jr., Fleischer, R. L. (1975) Apollo 17 cosmic-ray experiment - Interplanetary heavy nuclei of energies 0.05 to 5.0 MeV per atomic mass unit. The Astrophysical Journal, 198. 183pp. doi:10.1086/153591
	Lezniak, J. A., Webber, W. R. (1978) The charge composition and energy spectra of cosmic-ray nuclei from 3000 MeV per nucleon to 50 GeV per nucleon. The Astrophysical Journal, 223. 676pp. doi:10.1086/156301
	*Fleischer, R. L., Hart, H. R., Jr., Renshaw, A. (1974) Composition of heavy cosmic rays from 25 to 180 MeV per atomic mass unit. The Astrophysical Journal, 193. 575pp. doi:10.1086/153194*
	*Juliusson, Einar (1974) Charge Composition and Energy Spectra of Cosmic-Ray Nuclei at Energies above 20 GeV Per Nucleon. The Astrophysical Journal, 191. 331pp. doi:10.1086/152972*
	Binns, W. R., Garrard, T. L., Israel, M. H., Jones, Michael D., Kamionkowski, M. P., Klarmann, J., Stone, E. C., Waddington, C. J. (1988) Cosmic-ray energy spectra between 10 and several hundred GeV per atomic mass unit for elements from Ar-18 to Ni-28 - Results from HEAO 3. The Astrophysical Journal, 324. 1106pp. doi:10.1086/165966
	Orth, C. D., Buffington, A., Smoot, G. F., Mast, T. S. (1978) Abundances and spectra for cosmic-ray nuclei from lithium to iron for 2 to 150 GeV per nucleon. The Astrophysical Journal, 226. 1147pp. doi:10.1086/156692
	*Caldwell, J. H. (1977) Charge composition and energy spectra of cosmic-ray nuclei at energies above 5 GeV per nucleon. The Astrophysical Journal, 218. 269pp. doi:10.1086/155680*
	Grunsfeld, John M., L'Heureux, Jacques, Meyer, Peter, Muller, Dietrich, Swordy, Simon P. (1988) Energy spectra of cosmic-ray nuclei from 50 to 2000 GeV per AMU. The Astrophysical Journal, 327. doi:10.1086/185134

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Dwyer, R. (1978) The mean mass of the abundant cosmic-ray nuclei from boron to silicon at 1.2 GeV per atomic mass unit. The Astrophysical Journal, 224. 691pp. doi:10.1086/156417

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