Results 91 to 100 of about 652 (175)
Energetic neutral atom (ENA) observations provide valuable insights into the plasma conditions in the heliosphere and the surrounding interstellar medium.
Paweł Swaczyna +2 more
doaj +1 more source
Consequences of Hot Electrons for the Structure of the Outer Heliosphere
The temperature of electrons is largely unknown in the outer heliosphere because there is a gap in Voyager measurements from ∼3 eV to 22 keV. Most models assume that the electrons have the same temperature as the bulk cold thermal solar wind (10 ^4 K ...
Ethan Schuyler Bair +5 more
doaj +1 more source
Division II: Sun and Heliosphere (Soleil Et Heliosphere) [PDF]
openaire +1 more source
Dynamical Age of Alfvénic Turbulence in the Solar Wind
An evolving turbulent flow like the solar wind can be meaningfully characterized by its “turbulence age”—an estimate of the number of nonlinear times that have elapsed during the plasma’s propagation from the Sun to the point of observation.
Rohit Chhiber +3 more
doaj +1 more source
The structure of a complex, asymmetric coronal mass ejection revealed by 17 spacecraft across the inner heliosphere. [PDF]
Luspay-Kuti A +30 more
europepmc +1 more source
Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source
Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe. [PDF]
Brandt PC +42 more
europepmc +1 more source
IMAP's Role in Understanding Particle Injection and Energization Throughout the Heliosphere. [PDF]
Cohen CMS +30 more
europepmc +1 more source
Dust in and Around the Heliosphere and Astrospheres. [PDF]
Sterken VJ +9 more
europepmc +1 more source
Potential Solar Precursors to Magnetic Switchbacks. [PDF]
Tripathi D +11 more
europepmc +1 more source

