A glass acousto-optic deflector (AOD) is mounted in a 0.5 m spectrometer fo
r atomic emission background correction. The system allows sequential and r
apid observation of adjacent wavelengths for "on" and ''of" atomic line bac
kground correction. Particular attention is directed to optical masking and
data acquisition. While AOD components slightly degrade spectroscopic reso
lution, proper optical masking minimizes this problem and enhances AOD diff
raction efficiency. Conversely, reduction of light throughput by masking fo
rces a compromise in minimal useful aperture diameters. Representative atom
ic spectra with a neon hollow cathode lamp are presented. Utilizing appropr
iate AOD masking arrangements produced an increase in observed neon line wi
dths to 0.14 nm from the 0.09 nm widths observed in the absence of the AOD.
While the acousto-optic has the capability to alternate observed wavelengt
hs in the 100 kHz range, the 3000 Hz upper frequency limit is a function of
the current computer manipulation software. The best signal-to-noise ratio
s were obtained at higher sampling rates. Background correction was perform
ed with a microwave-induced plasma atomic emission source. Spectral charact
erizations were obtained with the 425 nm scandium emission line, the sodium
doublet near 589 nm and the chromium triplet in the 427 nm region. Calibra
tion plots were obtained with solution nebulization and electrothermal vapo
rization. Time-detector response profiles are illustrated for electrotherma
lly vaporized analytes.