Copyright © Philip M. Parker, INSEAD. Terms of Use.
| Domain | Definition |
Physics | The current at which radiation losses in a z pinch equilibrium (from bremsstrahlung and line radiation) are exactly balanced by the ohmic heating of the z pinch assuming classical (Spitzer-Harm) resistivity. If the current through a z pinch exceeds the Pease-Braginskii current, a rapid collapse of the z pinch can occur, which is known as radiative collapse. (references) |
Source: compiled by the editor from various references; see credits. | |
Crosswords: PEASE-BRAGINSKII CURRENT |
| Specialty definitions using "PEASE-BRAGINSKII CURRENT": Radiative Collapse. (references) |
Hexadecimal (or equivalents, 770AD-1900s) (references)50 45 41 53 45 2D 42 52 41 47 49 4E 53 4B 49 49 43 55 52 52 45 4E 54 |
| Leonardo da Vinci (1452-1519; backwards) (references)
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Binary Code (1918-1938, probably earlier) (references)01010000 01000101 01000001 01010011 01000101 00101101 01000010 01010010 01000001 01000111 01001001 01001110 01010011 01001011 01001001 01001001 00100000 01000011 01010101 01010010 01010010 01000101 01001110 01010100 |
HTML Code (1990) (references)P E A S E - B R A G I N S K I I   C U R R E N T |
ISO 10646 (1991-1993) (references)0050 0045 0041 0053 0045 002D 0042 0052 0041 0047 0049 004E 0053 004B 0049 0049 0043 0055 0052 0052 0045 004E 0054 |
Encryption (beginner's substitution cypher): (references)50393553391536523541434853454343237555252394854 |
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Copyright © Philip M. Parker, INSEAD. Terms of Use.
