activity
20172021
most citedAutomated Coronal Hole Identification via Multi-Thermal Intensity Segmentation

66 citations · 159 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2021★ 7 cited

Machine Learning Applications to Kronian Magnetospheric Reconnection Classification

Tadhg M. Garton, Caitriona M. Jackman, Andy W. Smith +3

The products of magnetic reconnection in Saturn's magnetotail are identified in magnetometer observations primarily through characteristic deviations in the north-south component o…

astro-ph.SR2021★ 34 cited

The Observational Uncertainty of Coronal Hole Boundaries in Automated Detection Schemes

Martin A. Reiss, Karin Muglach, Christian Möstl +16

Coronal holes are the observational manifestation of the solar magnetic field open to the heliosphere and are of pivotal importance for our understanding of the origin and accelera…

astro-ph.IM2020★ 32 cited

Integrating Machine Learning for Planetary Science: Perspectives for the Next Decade

Abigail R. Azari, John B. Biersteker, Ryan M. Dewey +13

Machine learning (ML) methods can expand our ability to construct, and draw insight from large datasets. Despite the increasing volume of planetary observations, our field has seen…

astro-ph.SR2018★ 20 cited

Expansion of High Speed Solar Wind Streams from Coronal Holes through the Inner Heliosphere

Tadhg M. Garton, Sophie A. Murray, Peter T. Gallagher

Coronal holes (CHs) are regions of open magnetic flux which are the source of high speed solar wind (HSSW) streams. To date, it is not clear which aspects of CHs are of most influe…

astro-ph.SR2017★ 66 cited

Automated Coronal Hole Identification via Multi-Thermal Intensity Segmentation

Tadhg M. Garton, Peter T. Gallagher, Sophie A. Murray

Coronal holes (CH) are regions of open magnetic fields that appear as dark areas in the solar corona due to their low density and temperature compared to the surrounding quiet coro…