Results 121 to 130 of about 10,278 (236)
Ground-based solar observations provide key contextual data (i.e., the 'big picture') to produce a complete description of the only astrosphere we can study in situ: our Sun's heliosphere.
Bain, Hazel M. +13 more
core
The Solar Orbiter mission – Exploring the Sun and heliosphere
Daniel Mueller +3 more
openalex +1 more source
The Sun as the Source of Nonlinear MHD Perturbations of the Solar Corona and the Heliosphere [PDF]
S. A. Grib
openalex +1 more source
Research on the interstellar medium and its interaction with the solar system constitutes a significant topic in planetary physics. As the Sun traverses the local interstellar cloud, interstellar neutrals penetrate the heliosphere, forming the ...
JiaLing Lyu +3 more
doaj +1 more source
Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere [PDF]
Yuming Wang +53 more
openalex +1 more source
Astrospheres and Solar-like Stellar Winds
Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the ...
Wood Brian E.
doaj
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
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
THE SUN AND THE HELIOSPHERE IN FEBRUARY-MARCH, 1986
Conditions of the sun and the heliosphere are studied in relation to the intense disturbances of the earth's and cometary magnetospheres in February and March, 1986. In this sunspot minimum phase, the sun had essentially the southward axial dipole which was to produce a weak northward IMF. However, one bipolar magnetic region in the northern hemisphere
openaire +1 more source
First Imaging of Coronal Mass Ejections in the Heliosphere Viewed from Outside the Sun – Earth Line
R. A. Harrison +15 more
openalex +2 more sources

