A machine learning based approach to active magnetic field cancellation
ORAL
Abstract
The Neutron Electric Dipole Moment experiment at the Spallation Neutron Source
(nEDM@SNS) is being commissioned to measure the nEDM to a precision of 1.6 ×
10-28 e·cm in the critical spin dressing mode. Achieving this level of precision
requires extreme control over magnetic fields in the measurement region, with
strict requirements on field gradients. The experiment features many layers of
passive magnetic shielding, including a superconducting lead shield. It is
important for there to be zero field inside the lead shield when it goes
superconducting, otherwise magnetic flux will be trapped. To aid in this, an active
magnetic field cancellation system will be used to monitor and cancel ambient
fields. A prototype system is being developed for the Systematics and Operational
Studies apparatus at the PULSTAR reactor (SOS@PULSTAR) at North Carolina
State University. SOS@PULSTAR provides a testbed for the nEDM@SNS
experiment, sharing many of the same design features but its smaller size allows
for more rapid warming/cooling cycles. The strict magnetic field uniformity
requirements for nEDM@SNS and SOS@PULSTAR prevent a magnetic field probe
from being placed inside the superconducting shield where the field needs to be
zeroed. To overcome this, a machine learning based method is being developed
where external sensors predict the field in the region of interest. This predicted
value can then be used as feedback for the active cancellation system.
(nEDM@SNS) is being commissioned to measure the nEDM to a precision of 1.6 ×
10-28 e·cm in the critical spin dressing mode. Achieving this level of precision
requires extreme control over magnetic fields in the measurement region, with
strict requirements on field gradients. The experiment features many layers of
passive magnetic shielding, including a superconducting lead shield. It is
important for there to be zero field inside the lead shield when it goes
superconducting, otherwise magnetic flux will be trapped. To aid in this, an active
magnetic field cancellation system will be used to monitor and cancel ambient
fields. A prototype system is being developed for the Systematics and Operational
Studies apparatus at the PULSTAR reactor (SOS@PULSTAR) at North Carolina
State University. SOS@PULSTAR provides a testbed for the nEDM@SNS
experiment, sharing many of the same design features but its smaller size allows
for more rapid warming/cooling cycles. The strict magnetic field uniformity
requirements for nEDM@SNS and SOS@PULSTAR prevent a magnetic field probe
from being placed inside the superconducting shield where the field needs to be
zeroed. To overcome this, a machine learning based method is being developed
where external sensors predict the field in the region of interest. This predicted
value can then be used as feedback for the active cancellation system.
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Presenters
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Matthew Morano
North Carolina State University
Authors
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Matthew Morano
North Carolina State University