Coronal structure and the solar windAspects concerning the open coronal structure and geomagnetic disturbances are considered along with the general coronal emission characteristics and relations between the open coronal structure and the interplanetary field. The nonstatistical indicators of coronal structure are examined and questions are investigated regarding the accuracy obtained in the determination of the emission latitude and longitude in the high corona for plasma, fields, and particles. Attention is given to the problem of particle population organization by low-coronal neutral line structures in the absence of a high coronal polarity structure.
Document ID
19750043936
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Roelof, E. C. (New Hampshire, University Durham, N.H., United States)