4 papers
Local Interstellar Flow Parameters from the First Intersection of IMAP-Lo's Parameter Tubes
Nathan A. Schwadron, Mitchell M. Shen, Fatemeh Rahmanifard +24
The Sun's motion through the interstellar medium creates a flow of interstellar neutral (ISN) atoms through the heliosphere. ISN He, due to its high universal abundance and relativ…
Ionization Rate of Interstellar Neutral Helium from New Horizons/SWAP Observations
MaÅgorzata Antonik, PaweÅ Swaczyna, David J. McComas +2
Interstellar neutral (ISN) atoms enable studies of the physical conditions in the local interstellar medium surrounding the heliosphere. ISN helium, which is the most abundant spec…
Production and Loss Processes of Hydrogen Energetic Neutral Atoms in the Heliosphere from 5 eV to 500 keV
PaweÅ Swaczyna, Maciej Bzowski, Marzena A. Kubiak
Energetic Neutral Atom (ENA) observations provide valuable insights into the plasma conditions in the heliosphere and the surrounding interstellar medium. Unlike plasma detectors,…
Global Heliospheric Termination Shock Strength in the Solar-Interstellar Interaction
E. J. Zirnstein, R. Kumar, B. L. Shrestha +4
A heliospheric termination shock (HTS) surrounds our solar system at approximately 100 astronomical units from the Sun, where the expanding solar wind (SW) is compressed and heated…