scholarly journals Organization of Energetic Particles by the Solar Wind Structure During the Declining to Minimum Phase of Solar Cycle 23

Solar Physics ◽  
2010 ◽  
Vol 263 (1-2) ◽  
pp. 239-261 ◽  
Author(s):  
C. O. Lee ◽  
J. G. Luhmann ◽  
I. de Pater ◽  
G. M. Mason ◽  
D. Haggerty ◽  
...  
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Energetic Particles ◽  
Minimum Phase ◽  
Wind Structure ◽  
Solar Cycle 23 ◽  
Solar Wind Structure

scholarly journals Solar cycle changes of large-scale solar wind structure

2009 ◽  
Vol 5 (S264) ◽  
pp. 356-358 ◽  
Author(s):  
P. K. Manoharan
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Large Scale ◽  
Interplanetary Space ◽  
The Sun ◽  
Wind Structure ◽  
Level Of Activity ◽  
Solar Wind Structure ◽  
Current Minimum ◽  
Inner Heliosphere

AbstractIn this paper, I present the results on large-scale evolution of density turbulence of solar wind in the inner heliosphere during 1985–2009. At a given distance from the Sun, the density turbulence is maximum around the maximum phase of the solar cycle and it reduces to ~70%, near the minimum phase. However, in the current minimum of solar activity, the level of turbulence has gradually decreased, starting from the year 2005, to the present level of ~30%. These results suggest that the source of solar wind changes globally, with the important implication that the supply of mass and energy from the Sun to the interplanetary space has significantly reduced in the present low level of activity.

Empirical inner boundary conditions and rotation rates for solar wind models

2021 ◽  
Author(s):  
Huw Morgan
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Boundary Conditions ◽  
Coronal Magnetic Field ◽  
Height Range ◽  
Rotation Rates ◽  
Wind Structure ◽  
Solar Wind Structure ◽  
Coronal Electron ◽  
Made In

<p>To date, the inner boundary conditions for solar wind models are either directly or indirectly based on magnetic field extrapolation models of the photosphere. Furthermore, between the photosphere and Earth, there are no other direct empirical constraints on models. New breakthroughs in coronal rotation tomography, applied to coronagraph observations, allow maps of the coronal electron density to be made in the heliocentric height range 4-12 solar radii (Rs). We show that these maps (i) give a new empirical boundary condition for solar wind structure at a height where the coronal magnetic field has become radial, thus avoiding the need to model the complex inner coronal magnetic field, and (ii) give accurate rotation rates for the corona, of crucial importance to the accuracy of solar wind models and forecasts.</p>

scholarly journals Relationship between Solar Energetic Particles and Properties of Flares and CMEs: Statistical Analysis of Solar Cycle 23 Events

Solar Physics ◽  
2015 ◽  
Vol 290 (3) ◽  
pp. 841-874 ◽  
Author(s):  
M. Dierckxsens ◽  
K. Tziotziou ◽  
S. Dalla ◽  
I. Patsou ◽  
M. S. Marsh ◽  
...  
Keyword(s):  
Statistical Analysis ◽  
Solar Cycle ◽  
Energetic Particles ◽  
Solar Energetic Particles ◽  
Solar Cycle 23

The Long Term Cosmic Ray Variation Relevant to Solar Wind Structure in the Outer Heliosphere

1990 ◽  
pp. 199-203
Author(s):  
M.V. Alania ◽  
R.G. Aslamazashvili ◽  
T.B. Bochorishvili ◽  
L.I. Dorman ◽  
R.T. Guschina ◽  
...  
Keyword(s):  
Solar Wind ◽  
Cosmic Ray ◽  
Outer Heliosphere ◽  
Wind Structure ◽  
Solar Wind Structure
Sign in / Sign up

Export Citation Format

Share Document