| Autor: |
E. E. Bloemhof, C. R. Gwinn, R. M. Danen |
| Rok vydání: |
1994 |
| Předmět: |
|
| Zdroj: |
Infrared Astronomy with Arrays ISBN: 9789401044660 |
| DOI: |
10.1007/978-94-011-1070-9_97 |
| Popis: |
We discuss some theoretical and practical considerations relating to achieving spatial resolution higher than ~ λ/D, the nominal diffraction-limited resolution of a telescope of diameter D. Although the Nyquist criterion is often invoked as a justification for choosing pixel scales in array cameras, higher sampling densities are favored for imaging at and somewhat beyond the diffraction limit. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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