Data for "The Nature of Right-handed Polarized Ion-scale Waves In the Near-Sun Solar Wind and Extended Solar Corona: the Antisunward Fast-Magnetosonic Whistler Wave or the Sunward Ion Cyclotron Wave?" by Shi et al.

<h2>The database includes all theoretical analysis results based on the linear model.</h2> <h2>Captions:</h2> <p><strong>data_fig1.mat</strong> file is used to plot Figure 1, which is the data of the instabilities driven by the interplay of the temperature anisotropy and relative streaming speed of the proton beam component.</p> <div>x_axis: X axis data, relative streaming speed</div> <div>y_axis: Y axis data, temperature anisotropy</div> <div>gamma_max: normalized growth rate \gamma, used in figure 1a</div> <div>frequency_max: normalized frequency f in the plasma frame, used in figure 1b</div> <div>theta_max: wave propagating angle \theta in the plasma frame , used in figure 1c</div> <div>ellip_max: ellipticity \epsilon in the plasma frame, used in figure 1d</div> <div>theta_max_sc: wave propagating angle \theta in the spacecraft frame , used in figure 1e</div> <div>ellip_max_sc: ellipticity \epsilon in the spacecraft frame, used in figure 1f</div> <div>&nbsp;</div> <div>&nbsp;</div> <p><strong>data_fig2.mat </strong>file is used to plot Figure 2, which is the data of the dependence of the instability in regime I on the relative steaming speed of the proton beam component.</p> <div>&nbsp;sICW_x_axis1: X axis data of figure 2a, normalized k&nbsp;</div> <div>&nbsp;sICW_y_axis1: Y axis data of figure 2a, relative streaming speed</div> <div>&nbsp;sICW_gamma_all: normalized growth rate \gamma of sunward ICW in k and relative steaming speed space, used in figure 2a</div> <div>&nbsp;sICW_x_axis2: X axis data of figure 2b-2e, normalized k</div> <div>&nbsp;sICW_frequency: normalized frequency f of sunward ICW, used in figure 2b</div> <div>&nbsp;sICW_gamma: normalized growth rate \gamma of sunward ICW, used in figure 2c</div> <div>&nbsp;sICW_etr_b: the energy transfer rate of proton beam, used in figure 2d</div> <div>&nbsp;sICW_etr_c: the energy transfer rate of proton core, used in figure 2e</div> <div>&nbsp;</div> <div>&nbsp;asICW_x_axis1: X axis data of figure 2f, normalized k&nbsp;</div> <div>&nbsp;asICW_y_axis1: Y axis data of figure 2f, relative streaming speed</div> <div>&nbsp;asICW_gamma_all: normalized growth rate \gamma of antisunward ICW in k and relative steaming speed space, used in figure 2f</div> <div>&nbsp;asICW_x_axis2: X axis data of figure 2g-2j, normalized k</div> <div>&nbsp;asICW_frequency: normalized frequency f of antisunward ICW, used in figure 2g</div> <div>&nbsp;asICW_gamma: normalized growth rate \gamma of antisunward ICW, used in figure 2h</div> <div>&nbsp;asICW_etr_b: the energy transfer rate of proton beam, used in figure 2i</div> <div>&nbsp;asICW_etr_c: the energy transfer rate of proton core, used in figure 2j</div> <div>&nbsp;</div> <div>&nbsp;</div> <p><strong>data_fig3.mat</strong> file is used to plot Figure 3, which is the data of the dependence of the instability in regime I on the temperature anisotropy of the proton core component.</p> <div>&nbsp;sICW_x_axis1: X axis data of figure 3a, normalized k&nbsp;</div> <div>&nbsp;sICW_y_axis1: Y axis data of figure 3a, temperature anisotropy of the proton core</div> <div>&nbsp;sICW_gamma_all: normalized growth rate \gamma of sunward ICW in k and temperature anisotropy of the proton core space, used in figure 3a</div> <div>&nbsp;sICW_x_axis2: X axis data of figure 3b-3e, normalized k</div> <div>&nbsp;sICW_frequency: normalized frequency f of sunward ICW, used in figure 3b</div> <div>&nbsp;sICW_gamma: normalized growth rate \gamma of sunward ICW, used in figure 3c</div> <div>&nbsp;sICW_etr_b: the energy transfer rate of proton beam, used in figure 3d</div> <div>&nbsp;sICW_etr_c: the energy transfer rate of proton core, used in figure 3e</div> <div>&nbsp;</div> <div>&nbsp;asICW_x_axis1: X axis data of figure 3f, normalized k&nbsp;</div> <div>&nbsp;asICW_y_axis1: Y axis data of figure 3f, temperature anisotropy of the proton core</div> <div>&nbsp;asICW_gamma_all: normalized growth rate \gamma of antisunward ICW in k and temperature anisotropy of the proton core space, used in figure 3f</div> <div>&nbsp;asICW_x_axis2: X axis data of figure 3g-3j, normalized k</div> <div>&nbsp;asICW_frequency: normalized frequency f of antisunward ICW, used in figure 3g</div> <div>&nbsp;asICW_gamma: normalized growth rate \gamma of antisunward ICW, used in figure 3h</div> <div>&nbsp;asICW_etr_b: the energy transfer rate of proton beam, used in figure 3i</div> <div>&nbsp;asICW_etr_c: the energy transfer rate of proton core, used in figure 3j</div> <div>&nbsp;</div> <div>&nbsp;</div> <p><strong>data_fig4</strong>.mat file is used to plot Figure 4, which is the data of the dependence of the wave frequency on the bulk flow speed.</p> <div>&nbsp;x_axis: X axis of figure 4, bulk flow speed.</div> <div>&nbsp;y_axis1: Y axis of figure 4a, normalized relative streaming speed of regime III and V</div> <div>&nbsp;y_axis2: Y axis of figure 4b, normalized relative streaming speed of regime I</div> <div>&nbsp;fVsw_fmw: the normalized frequency distributions in spacecraft frame of antisunward fast-magnetosonic whistler waves in regimes III and V, used in figure 4a</div> <div>&nbsp;fVsw_sic: the normalized frequency distributions in spacecraft frame of sunward ion cyclotron waves in regimes I, used in figure 4b</div> <div>&nbsp;fVsw_fmw_n1: spacecraft frequency of antisunward fast-magnetosonic whistler waves on the 1.5VA bulk flow speed, used in figure 4c</div> <div>&nbsp;fVsw_fmw_n2: spacecraft frequency of antisunward fast-magnetosonic whistler waves on the 2.5VA bulk flow speed, used in figure 4c</div> <div>&nbsp;fVsw_sic_n1: spacecraft frequency of sunward ion cyclotron waves on the 0.25VA bulk flow speed, used in figure 4c</div> <div>&nbsp;fVsw_sic_n2: spacecraft frequency of sunward ion cyclotron waves on the 0.5VA bulk flow speed, used in figure 4c</div> <div>&nbsp;fVsw_sic_n3: spacecraft frequency of sunward ion cyclotron waves on the 0.75VA bulk flow speed, used in figure 4c</div>