Table 1: SUMER observations of temporal series in polar coronal holes (PCHs).
Item Date Time Solar coordinate Wavelength used Detector Exposure
    UT x ( $^{\prime \prime }$), y ( $^{\prime \prime }$) (Å) and slit time (s)
PCH 1 20/10/1996 19:57-23:57 0, 909.75 N N IV 765 Å, Ne VIII 770 Å B 2 (1 $^{\prime \prime }$ $\times$ 300 $^{\prime \prime }$) 30
PCH 2a 25/02/1997 00:03-13:58 0, 950.25 S N IV 765 Å B 2 (1 $^{\prime \prime }$ $\times$ 300 $^{\prime \prime }$) 60
PCH 2b 21/02/1997 01:20-01:35 0, 984.75 S C III 977 Å B 6 (0.3 $^{\prime \prime }$ $\times$ 120 $^{\prime \prime }$) 15


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