List of presentations stimulating the discussion of the team during the in-person meetings in Bern.
1st in-person meeting: June 20-24, 2022, ISSI Bern, Switzerland
- J. Heerikhuisen, Structure of the heliosphere as a function of a variety of physical processes
- M. Kornbleuth, A comparison of the croissant-like and comet-like heliotail configuration resulting from different MHD models
- M. Kornbleuth, Effects of varying solar wind conditions in a steady state heliosphere
- P. Swaczyna, Interstellar parameters derived from ISN He observations by IBEX
- M. Opher, Discussion on the assumption on BU model and future development of the SHIELD model
- A. Galli, One solar cycle of heliosphere obervations with IBEX: Energetic neutral hydrogen atoms observed with IBEX-Lo from 10 eV to 2 keV
- K. Dialynas, On the properties of 0.11 keV to 344 MeV ion spectra in the inner heliosheath using regularizerd kappa distribution
- M. Kornbleuth, A comparison of the croissant-like and comet-like heliotail configuration resulting from MHD models in modeled ENA maps
- K. Dialynas, Gkioulidou et al. paper: differences between the 0.5-55 keV ENA measured spectra and corresponding spectra from models
- D. Koutroumpa, Inversion of SWAN Ly-alpha maps – deriving calibrated total ionization rates for ISN H atoms
- M. Bzowski, WawHelioGlow: the Warsaw model of the heliospheric backscatter glow and comparison with selected SWAN observations
- P. Swaczyna, Elastic and charge exchange collisions – the angular scattering of ISN atoms
- M. Bzowski, WawHelIon – the Warsaw heliospheric ionization model, with special emphasis on the evolution of the solar wind structure
- H.-R. Müller, Absorption of stellar Lyman-alpha by the heliospheric hydrogen wall
- I. Kowalska-Leszczyńska, Absorption of the Lyman-alpha profile line
- F. Rahamanifard, Effects of rafiation pressure on ISN H observations by IBEX. Simulating ISN H fluxes to be observed inside the heliosphere
- A. Galli, Summary of the findings from the Galli et al. 2019 paper ISN H IBEX-Lo observation paper
- P. Swaczyna, Bulk flow and distribution of ISN He at 100 au
- H.-R. Müller, Trajectory methods for neutral velocity distribution functions in the heliosphere
- M. Bzowski, Time- and solar distance evolution of ISN H in the heliosphere and PUI fluxes based on WTPM, WawHelIon and WawHelioUV
- P. Swaczyna, H PUI observed on SWAP/New Horizons
2nd in-person meeting: October 9-13, 2023, ISSI Bern, Switzerland
- M. Kornbleuth, Inferring the Interstellar Magnetic Field Direction from Energetic Neutral Atom Observations of the Heliotail
- J. Heerikhuisen, Hydrogen and Helium in the Solar Wind
- F. Fraternale, Global modeling of the SW-LISM interaction with kinetic neutral atoms: role of electrons, helium ions and effects on the neutrals distributions
- M. Kornbleuth, Probing the Length of the Heliospheric Tail with ENAs from 0.52-80 keV
- L. Dyke, Using trajectory methods to examine velocity distribution functions of primary interstellar neutral hydrogen in a time-dependent force environment
- H.-R. Müller, Neutral hydrogen velocity distribution functions at a r=100 au reference distance, obtained by trajectory methods
- P. Swaczyna, Discussion on the ISN H filtration in the various models vs. NH observations
- Chika Onobugo (M. Opher’s student), Effect of Turbulent Heliospheric Tail on capturing Heliopause
- Erick Powell (M. Opher’s student), Constraints on BISM from Lyman-alpha
- D. Koutroumpa, Heliospheric interface diagnostics with high-resolution X-ray spectroscopy using micro-calorimeters
- M. Bzowski, The Direction of the Flow of Interstellar Neutral H Based on Photometric Observations from SOHO/SWAN
- I. Kowalska-Leszczyńska, Response of the Ly-alpha glow on time-evolution of the ionization and solar Ly-alpha line intensity.
- A. Galli, New general paper incl. data release of all model-free ISN H maps for all years from 2009-2023
- F. Rahmanifard, The Effect of Angular Scattering Imposed by Charge Exchange and Elastic Collisions on Interstellar Neutral Hydrogen Atoms
- P. Swaczyna, Updated interstellar conditions from ISN helium observations
- H.-R. Müller, Update about absorption of stellar Ly-alpha radiation in the hydrogen wall (TBC)
- K. Dialynas, Anisotropies of 40-139 keV ions beyond the TS and in the VLISM: Implications for ion spectra beyond the HP
- F. Rahmanifard, Discussion of IBEX-Lo response to ISN H
- A. Galli, The anomalously low ISN H energy measured with IBEX-Lo