Upload
fay-francis
View
235
Download
0
Embed Size (px)
DESCRIPTION
Current Techniques cp-FTMW spectroscopy has been extended to the (sub)millimeter 1,2,3,4,5,6 Relies on expensive (sub)millimeter receivers FASSST technique uses time correlation to enable fast sweeping in the (sub)millimeter region 7,8,9,10 Used for full band scans in various experiments 1.Brown et al., Rev. Sci. Inst., Zaleski et al., J. Mol. Spec., Park at al., J. Chem. Phys., Steber et al., J. Mol. Spec., Gerecht at al., Opt. Express, Neill et al., Opt. Express, Petkie et al., Rev. Sci. Inst., Medvedev et al., J. Mol. Spec., Fortman et al., Ap. J., Medvedev et al., Opt. Lett., 2010
Citation preview
Fast Sweeping Direct Absorption (sub)Millimeter Spectroscopy
Based on Chirped Pulse Technology
Brian Hays1, Steve Shipman2, Susanna Widicus Weaver1
1. Emory University2. New College of Florida
Speeding up (sub)millimeter Spectroscopy
• Standard (sub)millimeter spectroscopy, lock-in detection, search problem
• Microwave spectroscopy 2-40 GHz (need R~2.5 x 106 )
• (sub)Millimeter wave spectroscopy 50-1000 GHz (need R~1.5 x 108 )
• We require a broadband but sensitive technique
Current Techniques• cp-FTMW spectroscopy has been extended to the
(sub)millimeter1,2,3,4,5,6
• Relies on expensive (sub)millimeter receivers• FASSST technique uses time correlation to enable
fast sweeping in the (sub)millimeter region7,8,9,10
• Used for full band scans in various experiments
1. Brown et al., Rev. Sci. Inst., 20082. Zaleski et al., J. Mol. Spec., 20123. Park at al., J. Chem. Phys., 20114. Steber et al., J. Mol. Spec., 20125. Gerecht at al., Opt. Express, 20116. Neill et al., Opt. Express, 2013
7. Petkie et al., Rev. Sci. Inst., 19978. Medvedev et al., J. Mol. Spec., 20049. Fortman et al., Ap. J., 201010. Medvedev et al., Opt. Lett., 2010
Fast Linear Frequency Sweeps
• Detect the time response of a frequency sweep
• Apply linear correction for the frequency calibration
• Detect with bolometer for high sensitivity
• Limited by the detector bandwidth (~500 kHz)
Experiment
Microwave Synth0 - 50 GHz
AWG0 – 5 GHz
LPF 0 – 5 GHz
DDG
10 MHz Rb Clock
Mixer
BPF 9.1 – 14.2 GHz
Preampx2
19
dB
Atten
uato
r
AMC x3-27Sample Cell
Detector
NI DigitizerComputer
50 GHz – 1 THz
600 Hz1.5 ms sweeps
Time response of bolometer
• Frequency sweep from 144100 to 146100 MHz
• 1.5 ms duration at a rate of 600 Hz
• 1,000,000 averages taken over an hour
• Sweep rate of 1.333 THz/s (1.333 MHz/µs)
Time response of bolometer
Time response of bolometer
Background subtracted response
Filter baseline
• Filter the Fourier transform using low pass, high pass, and notch filters
• Spline fit using masking
2nd derivative spectrum
Comparison with lock-in spectrum
• Compared to lock-in 2nd derivative lineshape
• Lock-in gives higher SNR, but sweep is faster
Higher Frequency, Faster Sweep
• Frequency sweep from 336300 to 340300 MHz
• 1.5 ms duration at a rate of 600 Hz
• 10,000 averages taken over five minutes
• Background subtracted, then differentiated
Higher Frequency, Faster Sweep
Background subtraction at very high frequency
High Frequency Data
• Frequency sweep from 889500 to 891000 MHz
• 1.5 ms duration at a rate of 600 Hz
• 10,000 averages taken over five minutes
• Background subtracted, not differentiated
Broadband at high frequencies
• Frequency sweep from ~826000 to ~835000 MHz
• 1.5 ms duration at a rate of 600 Hz
• 10,000 averages taken over five minutes
• Background subtracted, not differentiated
• Very fast sweep rate, 6 THz/s
Fast Sweep Direct Absorption
• Fast sweeping without the AWG
• For use in pulsed experiments
See Luyao Zou’s talk this afternoon
Radicals TH03
Conclusions
• Extension of broadband techniques into the (sub)millimeter for absorption spectroscopy
• The frequency agility using an AWG was combined with the sensitivity of a bolometer, to produce very fast and highly sensitive spectra
• Provides a solution for addressing the search problem in (sub)millimeter spectroscopy
Acknowledgements
• Widicus Weaver Lab• NSF #CHE-1150492• NSF #CHE-1404341