most citedCombined Surface Flux Transport and Helioseismic Far-side Active Region Model (FARM)

8 citations · 15 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR20248 cited

Combined Surface Flux Transport and Helioseismic Far-side Active Region Model (FARM)

Dan Yang, Stephan G. Heinemann, Robert H. Cameron +1

Maps of the magnetic field at the Sun's surface are commonly used as boundary conditions in space-weather modeling. However, continuous observations are only available from the Sun…

astro-ph.SR2024

The influence of different coronal hole geometries on simulations of coronal wave -- coronal hole interaction

I. Piantschitsch, J. Terradas, E. Soubrie +4

The geometry of a coronal hole (CH) affects the density profile of the reflected part of an incoming global coronal wave (CW). In this study, we perform for the first time magnetoh…

astro-ph.SR2024

On the Origin of the sudden Heliospheric Open Magnetic Flux Enhancement during the 2014 Pole Reversal

Stephan G. Heinemann, Mathew J. Owens, Manuela Temmer +12

Coronal holes are recognized as the primary sources of heliospheric open magnetic flux (OMF). However, a noticeable gap exists between in-situ measured OMF and that derived from re…

astro-ph.SR2024

Classification of Enhanced Geoeffectiveness Resulting from High-Speed Solar Wind Streams Compressing Slower Interplanetary Coronal Mass Ejections

Stephan G. Heinemann, Chaitanya Sishtla, Simon Good +2

High-speed solar wind streams (HSSs) interact with the preceding ambient solar wind to form Stream Interaction Regions (SIRs), which are a primary source of recurrent geomagnetic s…

astro-ph.SR2024

Unveiling the Journey of a Highly Inclined CME: Insights from the March 13, 2012 Event with 110 Longitudinal Separation

F. Carcaboso, M. Dumbovic, C. Kay +8

A fast and wide Coronal Mass Ejection (CME) erupted from the Sun on 2012-03-13. Its interplanetary counterpart was detected in situ two days later by STEREO-A and near-Earth spacec…

astro-ph.SR2023

Coronal Models and Detection of Open Magnetic Field

Eleanna Asvestari, Manuela Temmer, Ronald M. Caplan +11

A plethora of coronal models, from empirical to more complex magnetohydrodynamic (MHD) ones, are being used for reconstructing the coronal magnetic field topology and estimating th…