Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data
We present the thermal-magnetic relation in a simple, isolated sunspot deduced from the inversion of 1.56 μm spectropolarimetric data. Due to the high Zeeman sensitivity of the g = 3, Fe I 1.5648 μm line, we can study this relationship in the entire sunspot. An inversion technique based on response functions is used to derive various parameters
Mathew, S. K. et al.
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2002