January 23: Heliospheric Pattern Recognition
Space Physics Seminar
AGU Parker Lecture Rerun: Heliospheric Pattern Recognition
Thursday, January 23, 2014
725 Commonwealth Ave.
Refreshments at 3:30pm in CAS 500
Talk begins at 4:00pm in CAS 502
It is well known that patterns must be recognized before models can be built to aid in our understanding of complex systems. Pattern recognition is one of the pleasures of doing science. Foundational understanding rooted in pattern recognition in the heliospheric system was provided by Professor Parker, famously in the form of the Parker spiral describing the heliospheric magnetic field. Following in that tradition, our community has recognized a profusion of patterns on all scales in the heliosphere, from turbulent flux tubes to the shape of its outer boundaries. It is the magnetic (rather than gravitational) organization of space that affords this wide variety of pattern over a broad range of scales. Examples of the variety of patterns recognized at magnetospheric and heliospheric mesoscales will be presented. These involve magnetic reconnection, the structure of the heliospheric current sheet, the coronal hole boundary, and sources of slow solar wind. The primary tools used to recognize these patterns are observations of suprathermal electrons and magnetic fields. From these data one can recognize not only pattern but clues about origin.