Call for NAM session abstracts: “Magnetic Connectivity and Coronal Waves: From Chromosphere to Solar Wind”

We are pleased to invite abstracts for an upcoming session at NAM 2026: “Magnetic Connectivity and Coronal Waves: From Chromosphere to Solar Wind”. NAM will take place at the University of Birmingham from the 20th-24th of July. If you feel you can contribute to this session, please submit an abstract using the link below:

https://forms.cloud.microsoft/Pages/ResponsePage.aspx?id=z8oksN7eQUKhXDyX1VPp86dlj3dhFB5DvP5Qd06n7sBUQlMwVUJEM0ZBUVVOT0dSQkNJR1Y5TDdRWi4u

All submissions must be completed by 23:45 on the 2nd of April, 2026.

Session Abstract:

Magnetic Connectivity and Coronal Waves: From Chromosphere to Solar Wind

Abstract:

The solar corona is threaded with magnetohydrodynamic fluctuations propagating from the chromosphere to the heliosphere. Coronal wave phenomena, including EUV waves, Alfvénic fluctuations, shock fronts, and radio signatures, play roles in energy transport, particle acceleration, and solar-wind formation. Recent studies combining remote imaging and spectroscopy from SDO/AIA, IRIS, and Solar Orbiter (EUI, SPICE) with in-situ plasma and magnetic-field measurements from Parker Solar Probe (FIELDS, SWEAP) and Solar Orbiter (MAG, SWA), together with numerical modelling, have improved our ability to trace waves from the low corona into interplanetary space. Joint radio imaging from ground-based arrays such as LOFAR and spacecraft particle measurements show how shock-driven structures associated with coronal mass ejections accelerate energetic particles along open magnetic field lines, while detections of torsional Alfvénic motions using DKIST/Cryo-NIRSP support expectations for wave-mediated energy transport. Key challenges remain, including establishing robust magnetic connectivity between remote observations and in-situ sampling, quantifying wave evolution across the chromosphere–corona transition, and incorporating observational constraints into wave models. This session will bring together researchers working on remote sensing, in-situ measurements, and MHD modelling and connectivity frameworks to clarify the role of waves in heating the corona and establishing the solar-wind.

Organisers: Simon Daley-Yates, Thomas Howson, Anmol Kumar, Hemanthi Miriyala