Differences between revisions 2 and 4 (spanning 2 versions)
Revision 2 as of 2018-02-22 21:50:57
Size: 308
Comment:
Revision 4 as of 2018-02-23 03:34:07
Size: 1027
Comment:
Deletions are marked like this. Additions are marked like this.
Line 5: Line 5:
The fluctuation of the magnetic field gradient around the test masses is the main source of magnetic noise in KAGRA [1].
However, the gradient has not been directly measured so far though the fluctuation of the uniform field were measured [2,3].
Thus, the purpose of this project is to measure the gradient fluctuation or set an upper limit to it.
Line 8: Line 12:
1タスクの定義は1週間程度で終わらせることができる研究
Line 21: Line 25:
== Document == == References & Related Documents ==
[1] Magnetic noise calculation for BS (and ETM/ITM, PRM/SRM) [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=4459|JGW-T1504459]]

[2] Measurement of Schumann Resonance [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=5544|JGW-G1605544]]

[3] [[http://iopscience.iop.org/article/10.1088/1742-6596/716/1/012020/meta|Measurement of Schumann Resonance at Kamioka]]

Measurement of the magnetic field gradient at the KAGRA site

Project description

The fluctuation of the magnetic field gradient around the test masses is the main source of magnetic noise in KAGRA [1]. However, the gradient has not been directly measured so far though the fluctuation of the uniform field were measured [2,3]. Thus, the purpose of this project is to measure the gradient fluctuation or set an upper limit to it.


Project schedule and Task List


Result


Presentation


[1] Magnetic noise calculation for BS (and ETM/ITM, PRM/SRM) JGW-T1504459

[2] Measurement of Schumann Resonance JGW-G1605544

[3] Measurement of Schumann Resonance at Kamioka

KAGRA/Subgroups/DET/maggrad (last edited 2018-02-27 13:08:41 by TomofumiShimoda)