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Low power, hi-flux sources for SuperNova |
The SuperNova diffractometer has been designed around two low power consumption yet high intensity X-ray micro-sources.
Built in-house by Agilent, the Nova (Cu) and Mova (Mo) X-ray sources combine the latest in micro-focus X-ray tube technology with specially designed multilayer X-ray optics.
Of the orthogonal, double bounce design, these multilayer optics achieve the efficient capture and focusing of X-rays into a high purity and well shaped X-ray beam (140 microns for Nova, 180 microns for Mova).
In a dual wavelength SuperNova system the low divergence, high brilliance X-ray beams are arranged at a 21.5 degree offset to each other, such that both beams coincide at the centre of the goniometer where they are directed onto the crystal sample.
The SuperNova’s two X-ray sources are powered from a single software controlled generator unit. This high voltage (50kV), low power consumption unit provides up to 50W of power to each X-ray source and provides virtually instantaneous switching between Mo and Cu wavelengths. Wavelength switching is completely automatic and can be initiated either by the click of a software icon or by queued Mo and Cu experiments which can be run automatically back to back. |

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Source comparison
| Wavelength |
Molybdenum (Mo) |
Copper (Cu) |
| Power |
Up to 50W |
Up to 50W |
| Optics |
Multilayer optics |
Multilayer optics |
| Beam |
180 microns |
140 microns |
Find out more
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