Results 171 to 180 of about 2,118 (212)
A Geomagnetic Estimate of Heliospheric Modulation Potential over the Last 175 Years. [PDF]
Owens MJ +6 more
europepmc +1 more source
Evidence for small-scale torsional Alfvén waves in the solar corona. [PDF]
Morton RJ +5 more
europepmc +1 more source
Alfvén waves in the solar corona: resonance velocity, damping length, and charged particles acceleration by kinetic Alfvén waves. [PDF]
Ayaz S +4 more
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The Sun and Heliosphere at Solar Maximum
Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis.
J Geiss, D J Mccomas, R B Mckibben
exaly +8 more sources
The Sun, the Solar Wind, and the Heliosphere
This volume presents a concise, up-to-date overview of current research on the observations, theoretical interpretations, and empirical and physical descriptions of the Sun, the Solar Wind, and the Heliosphere, from the solar interior outward to the ...
Miralles, Mari Paz +1 more
exaly +3 more sources
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The Sun and the Heliosphere in Three Dimensions
Astrophysics and Space Science Library, 1986Section I: The Corona.- Coronal Magnetic Fields - a Mini Survey.- Origins of the Solar Wind in the Corona.- The Heliospheric Energy Source.- Coronal Spectroscopy and Imaging from Spartan during the Polar Passage of Ulysses.- The Structure and Rotation of the Solar Corona: Implications for the Heliosphere.- OVI Diagnostics of Solar Wind Generation ...
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The Sun and the Heliosphere as an Integrated System
Astrophysics and Space Science Library, 2004This book, for the first time, ties together physical processes across the full scale of the heliosphere. It is about the natural connections that exist between various parts of the system. Therefore, it is mainly cast in terms of those mechanisms and phenomena rather than individual missions in space.
exaly +2 more sources
Multi-Angle Viewing of the Sun and the Inner Heliosphere
AIP Conference Proceedings, 2003We describe the concept of a proposed mission, called Multi‐Angle Solar Sources Explorer (MASSE), that would observe the Sun and the inner Heliosphere from an orbit at 0.72 AU over all solar longitudes. It would, in coordination with observations from Earth’s side, investigate the sources of solar activity from their origin deep within the Sun, their ...
Alexander Ruzmaikin +1 more
exaly +2 more sources
2014
The Sun is our star. It provides the energy that makes life’s existence on Earth possible. The main zones of the observed Sun are the photosphere, chromosphere, and corona. Their composition, structure, and peculiarities are intrinsically related with the interior where nuclear fusion occurs. Solar activity includes an 11-year solar cycle and different
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The Sun is our star. It provides the energy that makes life’s existence on Earth possible. The main zones of the observed Sun are the photosphere, chromosphere, and corona. Their composition, structure, and peculiarities are intrinsically related with the interior where nuclear fusion occurs. Solar activity includes an 11-year solar cycle and different
openaire +1 more source

