NHMFL User Services

 
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Magneto-optics, Ultraviolet, Visible and Near Infrared

All of the sources and spectrometers at the NHMFL now are coupled to the experiment in the magnet via optical fibers. This allows the lasers and some of the spectrometers to remain in one place even though experiments are done in pulsed magnets, resistive magnets or superconducting magnets located at some distance. Experiments can be done at wide ranges of temperature and pressure. Similar capabilities exist in Los Alamos and Tallahassee.

Complete laser systems provide wavelengths from the near ultraviolet to the near infrared at both locations. Each includes a Coherent MIRA 900 dual mode locked Ti:Sapphire laser capable of operating in the pulsed (femtosecond or picosecond) or continuous wave modes, a 10 W argon laser to pump the Ti:Sapphire, and a 7 W, UV capable argon laser. The lasers have the following wavelengths: 351.1 nm (300 mW), 363.8 nm (300 mW), 488.0 nm (2.4 W), 514.5 nm (3.3 W), and a tunable band for the Ti:Sapphire (>=100 mW continuous wave output) of 700 - 1050 nm . The time scales of the Ti:S laser in modelocked operation are 130 fs and 2 ps, and the wavelength range is 720 nm to 1000 nm.

The following equipment is available for pulsed fields and in the 20 T superconducting magnet in Los Alamos:

Users of the resistive and superconducting magnets in Tallahassee have available a MacPherson 0.75 m single grating monochrometer/spectrometer. The accessories on hand provide 0.01 nm resolution and cover wavelengths from 300 to 900 nm (7 gratings). It is highly automated and features a UV coated 1024 X 256 CCD array detector for rapid spectroscopy in high fields (over 125 spectra in a single 3.5 hour shift).

The following other equipment is available for use in the resistive and superconducting magnets in Tallahassee:


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Curator: Scott Hannahs <sth@magnet.fsu.edu>
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