Radial nullness factors as du(f,du+2dr)=0, giving the two families. For r<b, u= constant has dr/dt=+f and is outgoing; du/dr=−2/f has dr/dt=−f and is ingoing. In the r,t∗=r+uplane they cross the horizon according to these slopes. The cosmological horizon prevents a future-directed inward lightsignal sent from r>b from reaching the static observer inside.