SDO/AIA observation in the 171 (left) and 304 (right) channels of the March 30 coronal rain event. AIA was roughly in quadrature with Solar Orbiter on this date. The large loop bundle observed in the AIA 171 map corresponds to the same loop bundle as was observed by HRI_EUV in Fig. 5. The dashed white-black paths follow some rain clumps observed in AIA 304. An animation corresponding to this figure is available online. The animation shows several rain clumps in AIA 304, but no clear counterpart is seen in AIA 171, although strong intensity variations are observed at the same locations. The animation runs from UT 00:02 to UT 00:49 and comprises the time where coronal rain is observed with HRI_EUV. It first runs without and then with the rain paths overlaid.