A Stand-Alone Surrogate Model for Predicting Protection Heater Delays in Nb3Sn Accelerator Magnets

Tutkimustuotos: ArtikkeliTieteellinenvertaisarvioitu

10 Lataukset (Pure)

Abstrakti

Quench is an irreversible transition where the magnet locally loses its superconducting properties and becomes resistive. Early quench detection and a prompt protection system response are essential to avoid conductor damage. One of the conventional methods for accelerator magnet quench protection is to place resistive heaters on the surface of the coils. The protection heaters are stainless steel strips which are powered with a voltage pulse from capacitor bank discharge. Current is passing through the heaters, generating heat due to the resistivity of the stainless steel. Heat is transferred to the cable by conduction. There is at least one layer of polyimide film and the cable insulation (impregnated glass fiber) between the heater and the superconducting cable. Heater delay is defined as the required time to reach the current sharing temperature in the cable after heater firing. Typically predicting the heater delay requires numerical simulations which are computationally somewhat challenging and require expertise and need of specific software. In this study, we are providing a fast and easily accessible surrogate model for predicting the heater delay in Nb 3 Sn magnets. Finite Element Method simulations with COMSOL Multiphysics are used for collecting the dataset and training a supervised artificial neural network algorithm. The model can be used for first estimations of heater delay in Nb 3 Sn accelerator magnets during their design phase. In future, the surrogate model could be also integrated with other quench protection design tools to accelerate the detailed protection design of future magnets.
AlkuperäiskieliEnglanti
Artikkeli4700806
JulkaisuIEEE Transactions on Applied Superconductivity
Vuosikerta35
Numero5
Varhainen verkossa julkaisun päivämäärä30 jouluk. 2024
DOI - pysyväislinkit
TilaJulkaistu - 2025
OKM-julkaisutyyppiA1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä

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