Modeling Magnetic Fields with Helical Solutions to Laplace’s Equation
ORAL
Abstract
The series solution to Laplace’s equation in a helical coordinate system is derived and refined using
symmetry and chirality arguments. These functions and their more commonplace counterparts are
used to model solenoidal magnetic fields via linear, multidimensional curve-fitting. A judicious
choice of functional forms, a small number of free parameters and sparse input data can lead to
highly accurate, fine-grained modeling of solenoidal magnetic fields, including helical features arising
from the winding of the solenoid, with overall field accuracy at better than one part per million.
symmetry and chirality arguments. These functions and their more commonplace counterparts are
used to model solenoidal magnetic fields via linear, multidimensional curve-fitting. A judicious
choice of functional forms, a small number of free parameters and sparse input data can lead to
highly accurate, fine-grained modeling of solenoidal magnetic fields, including helical features arising
from the winding of the solenoid, with overall field accuracy at better than one part per million.
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Presenters
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Cole Kampa
Northwestern University
Authors
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Brian Pollack
Northwestern University
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Ryan Pellico
Trinity College, Trinity College
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Cole Kampa
Northwestern University
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Henry Glass
Fermi National Accelerator Laboratory
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Michael Schmitt
Northwestern University