Fig. 1
Top: temporal evolution of a bright point in a quiet region (QR1). Columns display time series of SECCHI/EUVI images in λ30.4 nm (He ii), λ17.1 nm (Fe ix/x), and λ19.5 nm (Fe xii) and XRT images with Al_poly and Be_thin filters with 10 min intervals. Difference images are indicated by “diff” on columns. Dimension of the each panel is 100″ × 100″. Dotted lines on the XRT images mark the solar limb. Bottom: temporal evolution of a bright point in a coronal hole (CH1).
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