[PDF] Top 20 The origin and dynamic interaction of solar magnetic fields
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The origin and dynamic interaction of solar magnetic fields
... the magnetic field, plasma velocity and current, together with the vorticity, density and total pressure along a line (illustrated by the white line in Figure ... See full document
140
The investigation of quasi separatrix layers in solar magnetic fields
... of magnetic eld (up to several thousand Gauss) which inhibit heat ow to the surface from the convective zone ...At solar maximum there may be as many as 200 spots on the Sun's surface whereas at ... See full document
143
Solar wind electron interaction with the dayside lunar surface and crustal magnetic fields: Evidence for precursor effects
... the solar wind ...the solar wind frame than the dHT frame, indicating that it arises partly from reflection from a mov- ing obstacle, as also observed in the terrestrial foreshock (Fitzenreiter et ...crustal ... See full document
10
Origin of Magnetic Fields of Stellar Objects in the Universe Based on the 5D Projection Theory
... Thus, we consider that the generation of planets via the existence of the star sun is represented by the same group symmetry, and the 9 planets can be counted as 5 twins (with Pluto with its binary as a pair, but lying ... See full document
79
Solar Optical Telescope onboard Hinode for Diagnosing the Solar Magnetic Fields
... Figure 6 shows an example of SP data which is taken with the slit located on a quiet region near the disk center. From left to right shown the Stokes I, Q, U and V spec- tra; horizontal axis is wavelength covering two ... See full document
6
Magnetic flux transport simulations : applications to solar and stellar magnetic fields
... emerging magnetic flux on the solar surface is ...of magnetic flux on the solar ...the magnetic flux, especially the polar field, can vary greatly depending upon the peak value of ... See full document
176
Amplitude modulation of solar p-modes by surface magnetic fields
... real solar surface observations without further progress in the- ory (see ...of magnetic field and thermodynamic changes, the sound speed would need to be a function of wavenumber and frequency which is ... See full document
7
Fields, fractals and flares: characterising magnetic complexity in solar active regions
... weather, solar flares and coronal mass ejections, are thought to originate from active regions on the surface of the ...region magnetic fields on the ...Sun magnetic fields showed them ... See full document
176
The effects of magnetic fields on oscillations in the solar atmosphere
... This identification is also supported by an examination of the variation in amplitude of the surface modes, with distance from the interface. Miles and Roberts (1989a), following on from Roberts (1981a), have recently ... See full document
206
Fields and flares : understanding the complex magnetic topologies of solar active regions
... AR magnetic fields and ...LOS magnetic field observations during three X-class flares, and found changes in magnetic flux and transverse field due to the ...Sunspot magnetic field ... See full document
255
A Bcool survey of the magnetic fields of planet hosting solar type stars
... and magnetic interaction between host stars and their planets, especially large close-in “hot Jupiters”, has been of considerable interest since the discovery of such ...the magnetic activity of the ... See full document
16
A dynamic model of the eye nystagmus response to high magnetic fields
... high magnetic fields evoke nystagmus in human subjects with functioning vestibular ...involves interaction between ionic currents in the endolymph of the vestibular labyrinth and the static ... See full document
32
A BCool survey of the magnetic fields of planet-hosting solar-type stars
... made magnetic detections may be candidates for long-term magnetic topology mon- itoring (see Appendix ...the magnetic field of the host star may allow for modelling of the space weather environ- ment ... See full document
14
Evolution and characteristics of global pc5 ULF waves during a high solar wind speed interval
... of solar wind dynamic pressure (Figure 10a), Cluster magnetic fields and plasma measure- ments close to the magnetopause (Figure 10b), transverse magnetospheric magnetic and electric ... See full document
16
Magnetic fields on young, solar-type stars
... There are red giant branch (RGB) asymptotic giant branch (AGB) stars that are so- called “Lithium-rich” stars (Abia et al., 1999; Charbonnel and Balachandran, 2000). This would indicate that using the Li i 670.8 nm ... See full document
352
PG1258+593 and its common proper motion magnetic white dwarf counterpart
... strong magnetic field of SDSS J1300+5904 is related to the Ap phenomenon and not related to a com- mon envelope evolution, unless it is itself an unresolved bi- nary, or unrecognised ... See full document
8
Enhanced Phenomena in Metals with Electric and Magnetic Fields: II Magnetic Fields
... of interaction with external fields, that is, magnetization multiplied by field ...strong magnetic fields a larger number of precipitations and transformations are being ...Whilst magnetic fields are ... See full document
5
GUMICS 4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds
... their magnetic cloud ...2014, magnetic field magnitude measured by Cluster fluctuates as well prior to the ...2012 magnetic cloud event in both Cluster and Geo- tail ...reproduce magnetic ... See full document
19
Local Magnetoelectric Effect in La Doped BiFeO3 Multiferroic Thin Films Revealed by Magnetic Field Assisted Scanning Probe Microscopy
... quantum interference device (SQUID, Quantum Design). We used an atomic force microscopy (AFM) (NT-MDT Inc.) to characterize the surface topography, and the sur- face current distribution mapping was obtained by using the ... See full document
7
On Mars Thermosphere, Ionosphere and Exosphere: 3D Computational Study of Suprathermal Particles
... The spatial distribution of temperature averages and extrema, and the temperature structure in general, stays the same from the EL to the EH case (Figures 5.1a and 5.1b). However, the increase in the EUV flux leads to ... See full document
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