Differences between revisions 8 and 25 (spanning 17 versions)
Revision 8 as of 2016-08-05 09:47:14
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Revision 25 as of 2017-06-13 15:30:59
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== 7/1 Skype Telecon == == 7/1 2016 Skype Telecon ==
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== 7/8 in Sogang University == == 7/8 2016 in Sogang University ==
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== 8/2 Skype Telecon ==

== 8/2 2016 Skype Telecon ==
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== 8/4 ==
 * Parts arrived and some mechanical parts were wrong, but now they are fixed. JGP will assemble today.
== 8/4 2016 Skype telecon ==
 * The parts arrived; some mechanical parts were found wrong; JGP have fixed them; JGP will assemble today.
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 * KK will check the algorithm and will let you know today.  * KC made the new algorithm without arc tangent. JGP will check the formulas with real data. KK will check if it can be done in the CDS system or not.
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== 10/6 2016 skype telecon ==

 * Target is Physics Letter A.
 * To check the calibration again with the peak areas and higher harmonics taken into account.
 * To check the drift data with the calibration factor.
 * To check if the oplev noise went down or not after we took the tiltsensor out.
 * For paper, KK and SK will write the intro part, and JGP will write the resulting part.
 * Email to Kanda-san (KSC) about the open data

=== paper contents ===
 * we could calibrate oplev using the tilt sensor
 * They agreed ok
 * Tiltsensor's dynamic range was much larger than oplevs
 * environmental perturbation to be improved


== 10/20 2016 Local metting (KK & SJ) ==
 * We do not understand the calibration factors (or the spectrum magnitudes) change between tilt sensors and oplevs
 * We will re-center the MCE oplev on Monday
 * An excitation peak will be inserted on MCE and see if the peak height change in time
 * We will have another local meeting on Wednesday morning.

== 10/26 2016 skype meeting ==
 * oplev noise floor change of the last measurement is most likely because of the tilt sensor installation
 * Jungyu will come to KAGRA and we will repeat the measurement
 * Windshields will be available thanks to Akutsu san in the next measurement
 * Schedule is not fixed yet

== 3/1 2017 skype meeting ==
 * 2nd visit klog list http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/IOO/TiltSensor/Documents2
 * How can we proceed with KAGRA open data regulations?
    * Kawamura-sensei will contact to Kanda-san
    * Then Kokeyama will ask to KSC board
 * Paper contents
    * Comparison between oplev and tiltsensor spectra
    * present a cal peak to show tiltsensor is properly seeing the mirror motion
    * dark/ADC noise limit of tiltsensor
 * How can we estimate the tiltsensor dark or ADC noise limit?
    * Junegyu and Kyuman will study
 * Target is Optics Letters
 * Make a rough draft by Niigata f2f meeting
 * Next call will be a few days before f2f meeting for the presentation there

== 4/13 2017 skype meeting ==

MinutesMeeting0413

== 6/13 2017 skype meeting ==

 * Junegyu edit the draft by 6/14 evening
 * Seiji & Keiko will read by the end of this weekend (6/18)

Meeting

Note_First_Meeting

7/1 2016 Skype Telecon

  • KC and JGP will consider closer for the optical configuration (please upload new info)
  • KK will check if we have all necessary components
  • KK, KC and JGP will discuss about the disital software in Seoul
  • SK and KK will meet in Kamioka for a preparation (8/10)
  • We'll have another skype meeting before the site work

7/8 2016 in Sogang University

  • JGP will prepare the drawing of the configuration (on the pylon optical table)
  • JGP will prepare the required circuits (signal amps).
  • For the online data taking and analysis, we will need a digital model and MEDM screens. JGP will prepare the initial concept of the digital software.
  • With the prepared concept, we will build the model and make MEDM screens during KC/JGP visit (~1day).
  • We noticed that the digital software cannot do arc tangent. We will consider to use an approximation.
  • As planned, KK and SK will collect the necessary hardware on 8/10 (DC power supply, 50m cable, cable adaptors, AA filter)
  • KK will let JGP know about the Dsub 9 pin assignment to connect to an AA filter.

8/2 2016 Skype Telecon

Preparation

  • JGP will get the drawing in a few days.
  • All the parts will arrive today. KC and JGP will carry them (no shipping).
  • JGP will assemble and test the circuits this week. Reports will be made next week.
  • Model and MEDM screens will be prepared with Kirii-kun on 8/10 as well as the first phase of the visit.
  • KC will think about the approximation formula of art tangent to use in the digital model.
  • SJ will submit the "tunnel entrance form" for the experiment.
  • KK will send the Dsub pin assignment today.
  • KK will find AA filter soon.

Other note

  • No IR laser beam during the experiment.
  • We have to check again about the safety lecture.

Next meeting

  • Next meeting will be 8/5 9:20 am. KK will call everyone on skype.

8/4 2016 Skype telecon

  • The parts arrived; some mechanical parts were found wrong; JGP have fixed them; JGP will assemble today.
  • The drawing of the optical table (python table) will be done today by JGP.
  • Test result of the setup will be emailed.
  • KC made the new algorithm without arc tangent. JGP will check the formulas with real data. KK will check if it can be done in the CDS system or not.
  • Check the safety rule.
  • SJ will submit the mine entrance form.
  • JGP will carry the clumps (which is to fix the sensor on the table).

10/6 2016 skype telecon

  • Target is Physics Letter A.
  • To check the calibration again with the peak areas and higher harmonics taken into account.
  • To check the drift data with the calibration factor.
  • To check if the oplev noise went down or not after we took the tiltsensor out.
  • For paper, KK and SK will write the intro part, and JGP will write the resulting part.
  • Email to Kanda-san (KSC) about the open data

paper contents

  • we could calibrate oplev using the tilt sensor
  • They agreed ok
  • Tiltsensor's dynamic range was much larger than oplevs
  • environmental perturbation to be improved

10/20 2016 Local metting (KK & SJ)

  • We do not understand the calibration factors (or the spectrum magnitudes) change between tilt sensors and oplevs
  • We will re-center the MCE oplev on Monday
  • An excitation peak will be inserted on MCE and see if the peak height change in time
  • We will have another local meeting on Wednesday morning.

10/26 2016 skype meeting

  • oplev noise floor change of the last measurement is most likely because of the tilt sensor installation
  • Jungyu will come to KAGRA and we will repeat the measurement
  • Windshields will be available thanks to Akutsu san in the next measurement
  • Schedule is not fixed yet

3/1 2017 skype meeting

  • 2nd visit klog list http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/IOO/TiltSensor/Documents2

  • How can we proceed with KAGRA open data regulations?
    • Kawamura-sensei will contact to Kanda-san
    • Then Kokeyama will ask to KSC board
  • Paper contents
    • Comparison between oplev and tiltsensor spectra
    • present a cal peak to show tiltsensor is properly seeing the mirror motion
    • dark/ADC noise limit of tiltsensor
  • How can we estimate the tiltsensor dark or ADC noise limit?
    • Junegyu and Kyuman will study
  • Target is Optics Letters
  • Make a rough draft by Niigata f2f meeting
  • Next call will be a few days before f2f meeting for the presentation there

4/13 2017 skype meeting

MinutesMeeting0413

6/13 2017 skype meeting

  • Junegyu edit the draft by 6/14 evening
  • Seiji & Keiko will read by the end of this weekend (6/18)

KAGRA/Subgroups/IOO/TiltSensor/Meeting (last edited 2017-06-13 15:32:24 by KeikoKokeyama)