activity
20172026
most citedCharacteristics of Low-Latitude Coronal Holes near the Maximum of Solar cycle 24

59 citations · 176 across the 16 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

20 papers · 1 filter

astro-ph.SR2026

Coronal Mass Ejection and Heliospheric Current Sheet Interaction Causing a Long-Duration Magnetic Field Sector Transition

Manuela Temmer, Stephan G. Heinemann, Nina Dresing +2

We present a study that combines remote-sensing and in-situ observations of coronal mass ejections (CMEs) interacting with the nearby heliospheric current sheet (HCS). The sequence…

astro-ph.SR2025

CME Observations -- from Sun to Impact on Geospace

Manuela Temmer

Our Sun is an active star expelling dynamic phenomena known as coronal mass ejections (CMEs). The magnetic field configuration on the Sun and related solar wind structures affect t…

astro-ph.SR20241 cited

Deriving the interaction point between a Coronal Mass Ejection and High Speed Stream: A case study

Akshay Kumar Remeshan, Mateja Dumbovic, Manuela Temmer

We analyze the interaction between an Interplanetary Coronal Mass Ejection (ICME) detected in situ at the L1 Lagrange point on 2016 October 12 with a trailing High-Speed Stream (HS…

astro-ph.SR2024

Probing coronal mass ejections inclination effects with EUHFORIA

Karmen Martinić, Eleanna Asvestari, Mateja Dumbović +3

Coronal mass ejections (CMEs) are complex magnetized plasma structures in which the magnetic field spirals around a central axis, forming what is known as a flux rope (FR). The cen…

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.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…