Fig. 6

Directivity of the HXR emission calculated from Eq. (9) for electron energies of 30 keV, 50 keV, 100 keV and 200 keV for different models of electron energy losses and propagation directions. Solid line for CE model, dotted line for CB, and dashed line for CEB model. Propagation direction indicates the viewing angle for the observer looking from the top and varies from 0 to 90° for downwards emission and from 90° to 180° for upwards emission.
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