Comparing Automated Coronal Hole Detection Schemes with Coronal Magnetic Field Modeling

Karin Muglach; Reiss Martin; Satabdwa Majumdar; The S2-01 ISWAT Team

doi:https://doi.org/10.5194/egusphere-egu25-7810

[Back] [Session ST1.8]

EGU25-7810, updated on 14 Mar 2025

https://doi.org/10.5194/egusphere-egu25-7810

EGU General Assembly 2025

© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.

Comparing Automated Coronal Hole Detection Schemes with Coronal Magnetic Field Modeling

Karin Muglach¹, Reiss Martin², Satabdwa Majumdar³, and The S2-01 ISWAT Team

Karin Muglach et al.

¹NASA/GSFC, CUA, United States of America
²Community Coordinated Modelling Center, NASA Goddard Space Flight Center, Greenbelt, USA
³Austrian Space Weather Office, GeoSphere Austria, Graz, Austria

How to cite: Muglach, K., Martin, R., Majumdar, S., and S2-01 ISWAT Team, T.: Comparing Automated Coronal Hole Detection Schemes with Coronal Magnetic Field Modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7810, https://doi.org/10.5194/egusphere-egu25-7810, 2025.

This abstract has been withdrawn on 17 Apr 2025.