United Nations Security Council resolution | resolution | United Nations Security Council Resolution 1267 | United Nations Security Council Resolution 1373 | United Nations Security Council Resolution | Resolution (law) | Resolution | Image resolution | Gulf of Tonkin Resolution | Display resolution | United Nations Security Council Resolution 1559 | Optical resolution | Iraq resolution | HMS ''Resolution'' | Address Resolution Protocol | United Nations Security Council Resolution 418 | United Nations Security Council Resolution 1973 | United Nations Security Council Resolution 1822 | United Nations Security Council Resolution 1566 | United Nations Security Council Resolution 1484 | United Nations Security Council Resolution 1196 | United Nations Security Council Resolution 1170 | Springer resolution | Reverse Address Resolution Protocol | joint resolution | Iraq Resolution | HMS Resolution (Cook) | HMS Resolution | Final Resolution | Dispute Resolution |
The wide and general applicability of the Laplace transform and its inverse is illustrated by an application in astronomy which provides some information on the spatial distribution of matter of an astronomical source of radiofrequency thermal radiation too distant to resolve as more than a point, given its flux density spectrum, rather than relating the time domain with the spectrum (frequency domain).
The main scientific goal of the mission is the study of astronomical objects with an angular resolution up to a few millionths of an arcsecond.
He developed Lorentz STEM imaging, High Angular Resolution Electron Channeling X-ray Spectroscopy (HARECXS), High Angular Resolution Electron Channeling Electron Spectroscopy (HARECES), Position Resolved Diffraction, as well as his invention of the scanning confocal electron microscope and the π steradian Transmission X-ray Detector, for which he was given the R&D 100 Awards in 2003 and 2010 respectively.