In this overview map, all the debris clouds in my catalog are shown. Note, however, that many clouds have very few cataloged objects. This is especially true for high altitude clouds where the cloud may consistent of hundreds of significant-size debris objects only one or two of which are cataloged due to the limitations of current US Space Force sensors.
The main thing to notice here is how any given cloud generally covers only a fairly limited range of inclination. This is less true for high altitude clouds, since the lower velocities in high apogee orbits mean that a bigger inclination change happens for the same amount of delta-V.
In this map of low Earth orbit, we include clouds between 0 and 3000 km, and exclude clouds which extend to altitudes above 4000 km. Here it can be seen that the inclination ranges are usually very narrow for LEO debris clouds. This helps greatly with identifiying candidate parent clouds for a given debris object
This map shows only the largest debris clouds, those with more than 500 cataloged objects.
LEO Debris clouds with i between 60 and 80 degrees.
LEO Debris clouds with i between 80 and 97 degrees. Note the very localized cloud from the SNAPSHOT satellite ("SNAP")
LEO Debris clouds with i between 97 and 102 degrees, the main part of sun-synchrounous orbit, dominated by the FY-1C cloud but with many other debris clouds overlapping it. Note also the well-localized cloud from Nimbus 2 (NIM2) at 1100 km, 100.4 deg.
Large (more than 200 cataloged objects) LEO clouds in sun-synchronous orbit.
LEO Debris clouds with i between 99 and 105 degrees. Note the Delta 98/104/126 cloud, resulting from three Delta upper stage explosions, dominating the debris population above 101 deg.