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Pulsed Orotron—A new microwave source for submillimeter pulse high-field electron paramagnetic resonance spectroscopy
A vacuum-tube device for the generation of pulsed microwave radiation in the submillimeter range (up to 380 GHz ) is presented, designed for use as a source in a 360 GHz high-field/high-frequency electron paramagnetic resonance (EPR) spectrometer—the pulsed Orotron. Analogous to the known continuo...
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Published in: | Review of scientific instruments 2004-09, Vol.75 (9), p.2926-2936 |
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Main Authors: | , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | A vacuum-tube device for the generation of pulsed microwave radiation in the submillimeter range (up to
380
GHz
) is presented, designed for use as a source in a
360
GHz
high-field/high-frequency electron paramagnetic resonance (EPR) spectrometer—the pulsed Orotron. Analogous to the known continuous wave (cw) version, in the pulsed Orotron microwave radiation is generated by the interaction of a nonrelativistic electron beam with a diffraction grating (stimulated Smith–Purcell radiation) in feedback with an open Fabry–Pérot resonator construction. The presented design extends the cw Orotron by a gate electrode and a high-voltage pulsing unit to control the electron beam current. The generated pulses at
360
GHz
have pulse lengths from
100
ns
–10 μ
s
and a pulse power of
(22±5)
mW
. The output in a broader frequency band between 320 and
380
GHz
ranges from 20 up to
60
mW
. Within a
10 μ
s
time slot, incoherent pulse trains of arbitrary duration can be generated. The pulsed Orotron has been incorporated in the quasioptical microwave bridge of a heterodyne induction mode EPR spectrometer. The first free induction decay measurements at a microwave frequency of
360
GHz
and a magnetic field of
12.8
T
on a polycrystalline perylenyl–ion sample are presented and future applications and extensions of Orotron-EPR spectroscopy are discussed. |
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ISSN: | 0034-6748 1089-7623 |
DOI: | 10.1063/1.1778071 |