POLAR PLUME ANATOMY: RESULTS OF A COORDINATED OBSERVATION

• Main Authors: C. E. Deforest, J. T. Hoeksema, J. B. Gurman, B. J. Thompson, S. P. Plunkett, R. Howard, R. C. Harrison, D. M. Hassler Y
• Other Authors: The Pennsylvania State University CiteSeerX Archives
• Format: Text
• Language: English
• Published: 1997
• Subjects: South Pole; South pole
• Online Access: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.477.3879; http://www.boulder.swri.edu/~deforest/Papers_files/Sol Phys 1997 Deforest.pdf

Abstract. On 7 and 8 March 1996, the SOHO spacecraft and several other space- and ground-based observatories cooperated in the most comprehensive observation to date of solar polar plumes. Based on simultaneous data from five instruments, we describe the morphology of the plumes observed over the south pole of the Sun during the SOHO observing campaign. Individual plumes have been characterized from the photosphere to approximately 15 R, yielding a coherent por-trait of the features for more quantitative future studies. The observed plumes arise from small (2–5 arc sec diameter) quiescent, unipolar magnetic flux concentrations, on chromospheric net-work cell boundaries. They are denser and cooler than the surrounding coronal hole through which they extend, and are seen clearly in both Fe IX and Fe XII emission lines, indicating an ionization temperature between 1.0–1:5 106 K. The plumes initially expand rapidly with altitude, to a dia-meter of 20–30 Mm about 30 Mm off the surface. Above 1.2 R, plumes are observed in white light (as ‘coronal rays’) and extend to above 12 R. They grow superradially throughout their observed height, increasing their subtended solid angle (relative to disk center) by a factor of 10 between