Author: Maximenko, Y.B.
Paper Title Page
TUP041 Quench Dynamics in SRF Cavities: Can We Locate the Quench Origin with 2nd Sound? 883
 
  • Y.B. Maximenko
    MIPT, Dolgoprudniy, Moscow Region, Russia
  • D.A. Sergatskov
    Fermilab, Batavia, USA
 
  A newly developed method of locating quench in SRF cavities by detecting second-sound waves has been gaining popularity in SRF laboratories. The technique is based on measurements of time delays between the quench, as determined by the RF system, and arrival of the 2nd sound wave to the multiple detectors placed around the cavity in superfluid helium. Unlike multi-channel temperature mapping, this approach requires only few sensors and simple readout electronics; it can be used with SRF cavities of almost arbitrary shape. One of its drawbacks is that being an indirect method it requires one to solve an inverse problem to find a location of a quench. We tried to solve this inverse problem by using a parametric forward model. By analyzing the data we found that a simple model where 2nd-sound emitter is a near-singular source does not describe the physical system well enough. A time-dependent analysis of a quench process can help us to put forward a more adequate model. We present here our current algorithm to solve the inverse problem and discuss the experimental results.