Probing the effect of cadence on the estimates of photospheric energy and helicity injections in eruptive active region NOAA AR 11158
E. Lumme, M.D. Kazachenko, G.H. Fisher, B.T. Welsch, J. Pomoell,, E.K.J. Kilpua

TL;DR
This study investigates how the cadence of input data affects estimates of photospheric energy and helicity injections in an eruptive active region, finding that certain electric field methods are more stable across different cadences.
Contribution
The paper compares the stability of different electric field inversion methods across variable data cadences, introducing a novel DAVE4VM-based estimate that improves robustness.
Findings
PDFI method remains stable from 2.25 min to 2 hours cadence.
DAVE4VM estimates vary significantly with cadence.
A new DAVE4VM-based method reduces sensitivity to cadence.
Abstract
In this work we study how the input data cadence affects the photospheric energy and helicity injection estimates in eruptive NOAA active region 11158. We sample the novel 2.25-minute vector magnetogram and Dopplergram data from the \emph{Helioseismic and Magnetic Imager} (HMI) instrument onboard the \emph{Solar Dynamics Observatory} (SDO) spacecraft to create input datasets of variable cadences ranging from 2.25 minutes to 24 hours. We employ state-of-the-art data processing, velocity and electric field inversion methods for deriving estimates of the energy and helicity injections from these datasets. We find that the electric field inversion methods that reproduce the observed magnetic field evolution through the use of Faraday's law are more stable against variable cadence: the PDFI (PTD-Doppler-FLCT-Ideal) electric field inversion method produces consistent injection estimates for…
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