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The average line of sight component of this field has a strength of −0.6 ± 0.3 G.
a Full-disk image of a line-of-sight component of the solar magnetic field observed by SDO/HMI at 15:00 UT on 29 March 2014, which corresponds to 2.5 h before an X1.0-class flare.
A simple and intuitive analysis of that idea has shown that the relative altitude of the radar antenna location has a significant impact on receiving of a line-of-sight component of the backscatters (particularly in the case of a single target scenario).
Figure 2 a shows the line-of-sight component of the magnetic field, and the positive and negative polarities cover the whole sun. Figure 2 b shows the three-dimensional (3D) magnetic field lines traced from the positive to the negative polarities; these have been extrapolated under the assumption of the potential field approximation (this will be discussed below).
The ratio of the line of sight component to any of the other scatters is equal to k.
In addition, as described above, each radar gives only the line-of-sight component of drift velocity and the data are frequently missing.
where K is a Rician K-factor defined as the ratio of the powers of the line-of-sight components to the scattered components, γ 1 ¯ = Ω 1 γ 0 is the average SNR of the S1→Rlink, and I0is the zeroth order modified Bessel function of the first kind.
First, the line-of-sight component of ground displacement is retrieved via interferometric SAR (InSAR) analysis of pairs of SAR images spanning the eruption.
For the Rice MIMO channel, the channel matrix is (11). in which, K is the rice factor, HLOS and HRay are the line of sight component and the Rayleigh fading component of the channel matrix H, respectively.
Moreover, these derivations could, also, approximate that of the Rician channels when the mean channel matrix is of rank 1; this could be satisfied when all channel vectors have the same mean value or in some other practical scenarios where the line-of-sight (LOS) component of the channel matrix approaches the scaled all-ones matrix [37].
If ideally all LOSV measurements made for different beam directions scanned by various radars in a MLAT-MLT bin were their line-of-sight components of a single true flow vector, the LOSV value should be zero when the beam direction is exactly perpendicular to the true flow vector and the sign of LOSV flips across such an angle normal to the true flow.
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