ligo-g060410-00-z detchar introduction (8/16/06)k. riles - university of michigan 1 strainbandsmon...

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Detchar Introduction (8/16/06 ) K. Riles - University of Michigan 1 LIGO-G060410-00-Z StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan) (for Ramon Armen & Junyi Zhang) LIGO Scientific Collaboration Meeting LSU – August 16, 2006

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Page 1: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 1LIGO-G060410-00-Z

StrainBandsMon and SixtyHertzMon

Keith Riles (University of Michigan)

(for Ramon Armen & Junyi Zhang)

LIGO Scientific Collaboration MeetingLSU – August 16, 2006

Page 2: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 2LIGO-G060410-00-Z

StrainBandsMon(Ramon Armen)

E-mail from Rana last September (from Hannover):

Why doesn’t LIGO track band-limited RMS calibrated strain?

(the way GEO does)Ramon Armen (U. Michigan freshman) walked into my office about a week later to inquire about LIGO research opportunities

Over the next several months, Ramon dug into the DMT infrastructure (especially Patrick Sutton’s EasyCalibrate class) and created StrainBandsMon

Bingo!

Page 3: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 3LIGO-G060410-00-Z

StrainBandsMon

StrainBandsMon now running online:

And documented!

Produces status web page

Produces minute trends

Produces DMT viewer figure of merit

Page 4: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 4LIGO-G060410-00-Z

DMT Viewer Figure of Merit

Page 5: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 5LIGO-G060410-00-Z

Daily summaries(low frequency bands)

Page 6: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 6LIGO-G060410-00-Z

Daily summaries(high freq / broad / special bands)

Page 7: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 7LIGO-G060410-00-Z

Daily summaries(high freq / broad / special bands)

Link to status page

Link to documentation page

Page 8: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 8LIGO-G060410-00-Z

SixtyHertzMon(Junyi Zhang)

Idea:

Upconversion artifacts due to 60 Hz should track the slight frequency variations of power mains

Scheme:

1) Heterodyne DARM_ERR w.r.t. fixed 60 Hz signal (control)

2) Heterodyne DARM_ERR w.r.t, varying 60 Hz signal (frequency measured each minute from voltage monitor)

Compare spectra near 60 Hz (or higher harmonic) from 1) and 2):

If artifact is sharper in 2) than in 1), then 60 Hz is likely source

If artifact is sharper in 1) than in 2), 60 Hz source unlikely

Page 9: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 9LIGO-G060410-00-Z

Examples(S5 ±3Hz, ±6Hz)

63 Hz

54 Hz57 Hz

66 Hz

Page 10: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 10LIGO-G060410-00-Z

Examples(S4 120 Hz – short period)

Page 11: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 11LIGO-G060410-00-Z

Examples(S4 120 Hz – short period)

Page 12: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 12LIGO-G060410-00-Z

Suspicion: 78.6 = 18.6 Hz sideband on 60 Hz power mains (18.6 hz =beam splitter roll mode resonance)

1) is sharper than 2)

NOT 60 Hz sideband

Page 13: LIGO-G060410-00-Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)

Detchar Introduction (8/16/06) K. Riles - University of Michigan 13LIGO-G060410-00-Z

Status

• Program under active development

• Has been run on archived S4 & S5 data and on online data (fortress & marble)

• More infrastructure & documentation needed

• Plan to incorporate into online production following standard S5 protocol