Copyright © Philip M. Parker, INSEAD. Terms of Use.
| Domain | Definition |
Solar | A term for the amount of reflected radiation compared to the amount of incident radiation, or albedo, of a surface. The surface is not perfectly specular. That is, the reflected intensity is not at the same angle with respect to the surface normal as the incoming rays, nor are the two intensities necessarily equal (in crude terms, when light bounces off the Earth, some of it is absorbed and the rest of it bounces "funny", not as it would off a mirror). (references) |
Source: compiled by the editor from various references; see credits. | |
Hexadecimal (or equivalents, 770AD-1900s) (references)42 49 44 49 52 45 43 54 49 4F 4E 41 4C 52 45 46 4C 45 43 54 41 4E 43 45 |
| Leonardo da Vinci (1452-1519; backwards) (references)
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Binary Code (1918-1938, probably earlier) (references)01000010 01001001 01000100 01001001 01010010 01000101 01000011 01010100 01001001 01001111 01001110 01000001 01001100 00100000 01010010 01000101 01000110 01001100 01000101 01000011 01010100 01000001 01001110 01000011 01000101 |
HTML Code (1990) (references)B I D I R E C T I O N A L   R E F L E C T A N C E |
ISO 10646 (1991-1993) (references)0042 0049 0044 0049 0052 0045 0043 0054 0049 004F 004E 0041 004C 0052 0045 0046 004C 0045 0043 0054 0041 004E 0043 0045 |
Encryption (beginner's substitution cypher): (references)3643384352393754434948354625239404639375435483739 |
| 1. Orthography 2. Bibliography |
Copyright © Philip M. Parker, INSEAD. Terms of Use.
