The dispersions are calculated at different filling factors ν and different rs: (a) ν = 0, rs = 0.5, (b) ν = 0, rs = 1, (c) ν = 0, rs = 2, (d) ν = 1, rs = 0.5, (e) ν = 1, rs = 1, (f) ν = 1, rs = 2. Dispersions of 5 lowest-lying magnetoexciton states n2 → n1 indicated near the corresponding curves, are shown.
The results are presented for different filling factors ν and different rs: (a) ν = 0, rs = 0.5, (b) ν = 0, rs = 1, (c) ν = 0, rs = 2, (d) ν = 1, rs = 0.5, (e) ν = 1, rs = 1, (f) ν = 1, rs = 2. Dispersions of 3 lowest-lying magnetoplasmon modes n2 → n1, indicated near the corresponding curves, are shown.
The evolution of coronal mass ejection/shock system is investigated by numerically solving the usual set of two-dimensional single-fluid polytropic magnetohydrodynamic equations from 1 Rs to 1 AU in the meridian plane.
Each point for δB shown in Figs. 8, 9 and 10 is averaged within a small region of the magnetic latitude range Δθ = 0.1° with an equatorial radial distance range of ΔR = 1 Rs when Cassini passed through.
CMEs producing purely metric type II bursts are of lowest speed (611 km/s), which is sufficient to drive shocks near the Sun (within about 1 Rs from the surface).
A parallel adaptive mesh refinement (AMR) scheme for solving the governing equations of ideal magnetohydrodynamics (MHD) in three space dimensions is used herein to investigate the structure and evolution of a coronal mass ejection (CME) propagating from the solar surface at 1 Rs out into the inner heliosphere to distances approaching 12 AU.
[17] To determine the configuration and ee at C-1 of esters 6 and (S)- and (R -[D1] 6, they weR -[D1]ced witheyiAlH4 to diol - 7 and mixtures of diastereomeric diols (1 RS,2 R)- and (1 RS,2 S)-[2-D1] 7, respectively.
Most trenching treatments had significantly lower (by ∼0.5 μmol CO2 m−2 s−1) RS than the controls, and there was no significant difference in RS among the various trenching treatments.
Finally, Gas6 was strongly correlated with plasma concentrations of PCT (rs = 0.44, P = 0.005) and sTREM-1 (rs = 0.45, P = 0.003).
No correlation could be observed between platelet counts and Ang-1 (Rs = 0.1; P = 0.34) or Ang-2 (Rs = 0.1; P = 0.34) levels.
Furthermore, strong correlations were found between the levels of both uPA (rs = 0.85, P < 0.0001) and PAI-1 (rs = 0.90, P < 0.0001) in the cytosols and their levels previously measured with ELISAs based on commercial reagents.
