Table 1 Number of features nf detected in the time–distance diagrams by the computer vision technique

From: Observation of super-Alfvénic slippage of reconnecting magnetic field lines on the Sun

Intensity threshold (% of \({I}_{\max }\))

10

30

50

90

nf

\(\left\langle | {v}_{{\rm{slip}}}| \right\rangle\)

\({\sigma }_{| {v}_{{\rm{slip}}}| }\)

nf

\(\left\langle | {v}_{{\rm{slip}}}| \right\rangle\)

\({\sigma }_{| {v}_{{\rm{slip}}}| }\)

nf

\(\left\langle | {v}_{{\rm{slip}}}| \right\rangle\)

\({\sigma }_{| {v}_{{\rm{slip}}}| }\)

nf

\(\left\langle | {v}_{{\rm{slip}}}| \right\rangle\)

\({\sigma }_{| {v}_{{\rm{slip}}}| }\)

SJI 1,330

112

1,198

1,045

67

1,058

835

53

1,096

1,025

29

1,122

1,401

AIA 304

25

358

690

21

94

60

16

89

63

11

96

48

AIA 1,600

12

9

11

8

16

15

9

9

7

1

4

-

SJI d. TRACE (2 s)

95

2,291

1,298

60

1,943

1,209

43

1,969

1,304

29

2,295

1,780

SJI d. HI1

92

472

494

65

272

218

40

360

333

24

315

376

SJI d. HI2

34

96

85

38

158

378

29

89

83

20

92

75

  1. Average kernel velocities \(\left\langle | {v}_{{\rm{slip}}}| \right\rangle\) and the standard deviations \({\sigma }_{| {v}_{{\rm{slip}}}| }\) (in kilometres per second), calculated using the average orientation of the detected features, are indicated. Different columns of the table designate the three quantities determined using time–distance diagrams saturated to selected intensity thresholds (10–90% of the maximal intensity \({I}_{\max }\)).