How is the energy distributed in these modes?
How do they interact?
How do we find them?
The Karhunen-Loeve Transform can help answer these questions. It has several nice properties which can be exploited to determine a set of orthogonal spatial modes of the system and determine a measure of the energy contained within each mode.
Eigenfunction Analysis of Coherent Structures on the Solar Surface
Authoring NASA Official:Dr. Milton Halem, Chief, Earth
and Space Data Computing Division
Contact:Marilyn Mack/Code 930
marilyn.j.mack.1@gsfc.nasa.gov