Copyright © Philip M. Parker, INSEAD. Terms of Use.
| Domain | Definition |
Aerospace | The positively charge nuclei of elements heavier than hydrogen and helium up to atomic nuclei of iron. See cosmic rays.These heavy atomic nuclei comprise about 1 percent of the total cosmic-ray particles and less than 4 percent of the total positive charges. (references) |
Source: compiled by the editor from various references; see credits. | |
Hexadecimal (or equivalents, 770AD-1900s) (references)48 45 41 56 59 43 4F 53 4D 49 43 2D 52 41 59 50 52 49 4D 41 52 49 45 53 |
| Leonardo da Vinci (1452-1519; backwards) (references)
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Binary Code (1918-1938, probably earlier) (references)01001000 01000101 01000001 01010110 01011001 00100000 01000011 01001111 01010011 01001101 01001001 01000011 00101101 01010010 01000001 01011001 00100000 01010000 01010010 01001001 01001101 01000001 01010010 01001001 01000101 01010011 |
HTML Code (1990) (references)H E A V Y   C O S M I C - R A Y   P R I M A R I E S |
ISO 10646 (1991-1993) (references)0048 0045 0041 0056 0059 0043 004F 0053 004D 0049 0043 002D 0052 0041 0059 0050 0052 0049 004D 0041 0052 0049 0045 0053 |
Encryption (beginner's substitution cypher): (references)42393556592374953474337155235592505243473552433953 |
| 1. Orthography 2. Bibliography |
Copyright © Philip M. Parker, INSEAD. Terms of Use.
