Figures for ``Observation of Polar Plumes at High Solar Altitudes''

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Figure 1: Polar plumes extending from the surface of the Sun out to 30 R above the surface (in the image plane). This image is in conformal azimuthal coordinates. Vertical lines in the image represent radial lines in normal space, and the radial direction is scaled logarithmically. Four instruments' data are presented. The C-3, HAO K-coronameter, and EIT images have been smoothed and detrended as described in the text. The C-2 image has been subjected only to radial filtering, to demonstrate by coalignment that the C-3 features are solar and not artificial.
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Figure 2: The outermost (C3) portion of Figure 1, transformed back into normal image coordinates. This is a processed, radially-filtered image of the top half of the C-3 field of view, showing the actual appearance of the plumes as radial structures.
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Figure 3: Plot of measured LASCO image intensity (in digitizer counts per pixel per second) versus azimuth for several altitudes in Figure 2. The plots are centered on zero because the data are unsharp masked. At the highest plotted image-plane altitude (25 R), the plume-interplume contrast is approximately 0.2 count sec-1 pixel-1 peak to peak (0.07 count sec-1 pixel-1 RMS).
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Figure 4: Plots of intensity and flow-normalized intensity measured at the LASCO focal plane, versus altitude in several of the plumes in Figure 2. The flow-normalized intensity has been multiplied by b3 (the cube of the image-plane altitude) to remove the effects of illumination and rarefaction in a constant-speed, radial geometry wind.
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Figure 5: Geometry of a radially expanding plume, used in the derivation of equations (1) and (2) in the text. Plumes tilted out of the plane of the sky are seen at higher altitudes than is apparent on the film plane, an effect that is partially cancelled out by the thicker cross-section of the tilted plume along the line of sight.
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