Copyright © Philip M. Parker, INSEAD. Terms of Use.
| Domain | Definition |
Aerospace | Primary cosmic rays from outer space which consist mainly of protons with energies of 2-20 billion electron volts (Bev).For 1000 protons there are about 80 helium nuclei, about 3 nuclei in the carbon-nitrogen-oxygen range, and 1 or 2 heavier nuclei. The proton energy may be as high as 105 Bev, and the other nuclei show an energy distribution similar to that of the protons. (references) |
Source: compiled by the editor from various references; see credits. | |
Crosswords: CORPUSCULAR COSMIC RAYS |
| Specialty definitions using "CORPUSCULAR COSMIC RAYS": cosmic rays. (references) |
Hexadecimal (or equivalents, 770AD-1900s) (references)43 4F 52 50 55 53 43 55 4C 41 52 43 4F 53 4D 49 43 52 41 59 53 |
| Leonardo da Vinci (1452-1519; backwards) (references)
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Binary Code (1918-1938, probably earlier) (references)01000011 01001111 01010010 01010000 01010101 01010011 01000011 01010101 01001100 01000001 01010010 00100000 01000011 01001111 01010011 01001101 01001001 01000011 00100000 01010010 01000001 01011001 01010011 |
HTML Code (1990) (references)C O R P U S C U L A R   C O S M I C   R A Y S |
ISO 10646 (1991-1993) (references)0043 004F 0052 0050 0055 0053 0043 0055 004C 0041 0052 0043 004F 0053 004D 0049 0043 0052 0041 0059 0053 |
Encryption (beginner's substitution cypher): (references)37495250555337554635522374953474337252355953 |
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Copyright © Philip M. Parker, INSEAD. Terms of Use.
