Results 111 to 120 of about 2,118 (212)
Division II: The Sun and Heliosphere: (Soleil Et Heliosphere) [PDF]
Arnold O. Benz +6 more
openaire +1 more source
The Solar and Heliosphere Observatory (SOHO) website provides an overview of the SOHO mission, the instruments involved, the operations of the mission, and the latest articles about the mission.
core
Ion-scale Turbulence and Energy Cascade Rate in the Solar Corona and Inner Heliosphere
Plasma turbulence cascading from MHD to kinetic scales in the heliospheric plasma is believed to play a key role in coronal heating and fast solar wind acceleration, but the properties of the turbulence remain poorly constrained by observations.
Eduard P. Kontar +3 more
doaj +1 more source
Driving Dynamical Inner‐Heliosphere Models With In Situ Solar Wind Observations
Accurately reconstructing the solar wind throughout the inner heliosphere is essential for understanding solar–terrestrial interactions and improving space‐weather forecasts.
M. J. Owens +10 more
doaj +1 more source
This report covers technical progress during the fourth quarter of the second year of NASA Sun-Earth Connections Theory Program (SECTP) contract 'The Structure and Dynamics of the Solar Corona and Inner Heliosphere,' NAS5-99188, between NASA and Science ...
Grebowsky, Joseph +2 more
core
THE SUN AND THE HELIOSPHERE IN FEBRUARY-MARCH, 1986 [PDF]
1989-11Conditions 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
Saito, Takao, Oki, Tosio
core
Simulating a Steady-state Heliosphere
Ever since the discovery of the solar wind, it has been understood that our solar system resides within a bubble of solar wind plasma that originates from the Sun.
Jacob Heerikhuisen +2 more
doaj +1 more source
Manifestation of the stellar wind cycle in infrared images: Example of the heliosphere
Aims. The regions in which stellar winds interact with the interstellar medium, also known as astrospheres, can be observed in detail through the thermal emission of the interstellar dust particles, resided in plasma.
V. V. Izmodenov, I. P. Zabolotnyi
core +1 more source
Interstellar gas in the heliosphere and the solar wind anisotropies
International audienceA critical review of the interstellar hydrogen in the heliosphere will be presented. Recent Sun-interstellar matter interaction model improvements, a non-stationary flow and a flexible latitude dependence, will be discussed. We also
Lallement, Rosine +2 more
core +1 more source
The Vigil Magnetometer for Operational Space Weather Services From the Sun‐Earth L5 Point
Severe space weather has the potential to cause significant socio‐economic impact and it is widely accepted that mitigating this risk requires more comprehensive observations of the Sun and heliosphere, enabling more accurate forecasting of significant ...
J. P. Eastwood +12 more
doaj +1 more source

