Top panels: the intensity for heliospheric (left panel) and galactic (right panel) particles for three different choices of the pitch angle along a cut perpendicular to the HP. The four bottom panels show the distribution of heliospheric (panels a) and b)) and galactic (panels c) and d)) particles as a function of pitch angle at x = −2 AU (panels a) and c)) and x = 2 AU (panels b) and d)), with the arrow indicating the orientation of B. The normalized pitch-angle distributions are scaled differently in each panel, as indicated.