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Table 1

Observed periods and projected propagation speeds for all the slits marked in Fig. 1, in both 171 Å  and 193 Å.

Fe ix  171 Å Fe xii  193 Å

Slit No. P1(P2) Speed P1(P2) Speed
(min) (km s-1) (min) (km s-1)

1 24.3 (13.2) 103.2 ± 1.4 28.8 (12.1) 133.1 ± 2.3
2 18.7 (12.1) 113.8 ± 1.4 20.4 (17.1) 140.2 ± 2.3
3 31.4 (13.2) 110.9 ± 1.5 26.4 (13.2) 124.2 ± 1.6a
4 18.7 (11.1) 117.5 ± 1.9 22.2 (10.2) 142.2 ± 3.2b
5 28.8 (14.4) 109.9 ± 1.6 26.4 (10.2) 137.6 ± 2.5
6 26.4 (12.1) 116.5 ± 1.7 24.3 (17.1) 132.6 ± 1.9
7 28.8 (18.7) 121.5 ± 2.1 31.4 (17.1) 136.9 ± 3.4

μ ± σ 113.4 ± 5.6 135.2 ± 5.6
±δ ±0.6 ±0.9

8 24.3 (14.4) 137.4 ± 2.3 24.3 (14.4) 149.8 ± 2.6a
9 26.4 (17.1) 142.5 ± 1.8a 26.4 (18.7) 164.7 ± 2.9a
10 18.7 (12.1) 144.9 ± 2.7b 18.7 (11.1) 153.9 ± 3.6b
11 24.3 (...) 127.2 ± 1.6a 22.2 (...) 167.4 ± 3.8a
12 20.4 (13.2) 121.2 ± 2.1 28.8 (15.7) 165.1 ± 3.9

μ ± σ 134.6 ± 9.1 160.2 ± 7.0
±δ ±0.9 ±1.5

Notes. P1 and P2 are the primary and secondary periods (see Fig. 3). μ is the average of all the values above, σ is the standard deviation representing statistical error, and δ is the instrumental uncertainty propagated from individual values.

(a)

Jet-like features that can be seen from the movies.

(b)

Enhanced intensity regions showing a decelerating ridge at the end of space-time map. This is due to some eruption from a region above slits 4 and 10.

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