Towards Improved Heliosphere Sky Map Estimation with Theseus
Dave Osthus, Brian P. Weaver, Lauren J. Beesley, Kelly R. Moran,, Madeline A. Ausdemore, Eric J. Zirnstein, Paul H. Janzen, Daniel B., Reisenfeld

TL;DR
This paper introduces Theseus, a two-stage method for creating higher-resolution, less biased heliosphere sky maps from IBEX data, addressing noise, irregular sampling, and instrument PSF effects.
Contribution
Theseus is a novel two-stage approach combining ensemble regression and deconvolution, improving sky map estimation over existing methods.
Findings
Theseus outperforms current methods on simulated data.
It provides more accurate and higher-resolution sky maps.
Uncertainty estimates are effectively computed via bootstrapping.
Abstract
The Interstellar Boundary Explorer (IBEX) satellite has been in orbit since 2008 and detects energy-resolved energetic neutral atoms (ENAs) originating from the heliosphere. Different regions of the heliosphere generate ENAs at different rates. It is of scientific interest to take the data collected by IBEX and estimate spatial maps of heliospheric ENA rates (referred to as sky maps) at higher resolutions than before. These sky maps will subsequently be used to discern between competing theories of heliosphere properties that are not currently possible. The data IBEX collects present challenges to sky map estimation. The two primary challenges are noisy and irregularly spaced data collection and the IBEX instrumentation's point spread function. In essence, the data collected by IBEX are both noisy and biased for the underlying sky map of inferential interest. In this paper, we present a…
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Taxonomy
TopicsSolar Radiation and Photovoltaics · Solar and Space Plasma Dynamics · Adaptive optics and wavefront sensing
