dcterms created equal to or less than 2018-08-27T18:52:20.000Zequal to or more than 2018-08-27T18:52:20.000Z
dcterms modified equal to or less than 2020-11-03T20:03:20.134Zequal to or more than 2020-11-03T20:03:20.134Z
broader original
1910 original
definition A mathematical operation that allows to restore the original input signal, such as an astronomical image or spectrum, to its state before being affected by the atmospheric turbulence and the transfer function of the instrument.
Resource original
Concept original
contributor AAS_Frey.Katie original
creator AAS_Frey.Katie original