Copyright © Philip M. Parker, INSEAD. Terms of Use.
| Domain | Definition |
Nuclear Energy & Physics | A magnetohydrodynamic instability which can develop in a plasma column carrrying a strong axial current. When a constriction of the column begins to develop the magnetic field becomes st ronger which further constricts the plasma, possibly even leading to current interruption. Source: European Union. (references) |
Source: compiled by the editor from various references; see credits. | |
Hexadecimal (or equivalents, 770AD-1900s) (references)4E 45 43 4B 49 4E 47 2D 4F 46 46 49 4E 53 54 41 42 49 4C 49 54 59 |
| Leonardo da Vinci (1452-1519; backwards) (references)
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Binary Code (1918-1938, probably earlier) (references)01001110 01000101 01000011 01001011 01001001 01001110 01000111 00101101 01001111 01000110 01000110 00100000 01001001 01001110 01010011 01010100 01000001 01000010 01001001 01001100 01001001 01010100 01011001 |
HTML Code (1990) (references)N E C K I N G - O F F   I N S T A B I L I T Y |
ISO 10646 (1991-1993) (references)004E 0045 0043 004B 0049 004E 0047 002D 004F 0046 0046 0049 004E 0053 0054 0041 0042 0049 004C 0049 0054 0059 |
Encryption (beginner's substitution cypher): (references)483937454348411549404024348535435364346435459 |
| 1. Orthography 2. Bibliography |
Copyright © Philip M. Parker, INSEAD. Terms of Use.
