Statistical seismology of transverse waves in the solar corona

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Table 1

Characteristics of observed TLOs.

#	P (s)	τ (s)	L(Mm)	Reference¹

1	261	870	168	A02
2	265	300	72
3	316	500	174
4	277	400	204
5	272	849	162
6	435	600	258
7	143	200	166
8	423	800	406
9	185	200	192
10	396	400	146

11	234	714	350 ± 50	WS04

12	249 ± 33	920 ± 360	218	V04
13	448 ± 18	1260 ± 500	218
14	392 ± 31	1830 ± 790	228
15	382 ± 12	1330 ± 528	233
16	358 ± 30	1030 ± 570	237
17	326 ± 45	980 ± 400	235
18	357 ± 89	1320 ± 720	236

19	567	1500	400 ± 100	H05 & H07
20	918	4200	800 ± 200

21	425	2300	384	VD07
22	436 ± 4.5	2129 ± 280	400 ± 40
23	243 ± 6.4	1200	400 ± 40

24	895 ± 2	521 ± 8	228	DMB07 & VD09
25	452 ± 1	473 ± 6	228

26	630 ± 30	1000 ± 300	340 ± 15	V09

27	2418 ± 5	3660 ± 80	680 ± 50	V10

28	377	500	250	M11

29	225 ± 40	240 ± 45	121 ± 12	WV12
30	215 ± 5	293 ± 18	111 ± 11
31	213 ± 9	251 ± 36	132 ± 13
32	216 ± 27	230 ± 23	113 ± 11
33	520 ± 5	735 ± 53	396 ± 40
34	596 ± 50	771 ± 336	374 ± 37
35	212 ± 20	298 ± 30	279 ± 28
36	256 ± 22	444 ± 105	240 ± 24
37	135 ± 9	311 ± 85	241 ± 24
38	115 ± 2	175 ± 30	159 ± 16
39	103 ± 8	242 ± 114	132 ± 13

40	302 ± 14	306 ± 43	466 ± 50	W12

41	565 ± 4	666 ± 42	301 ± 30	V12
42	222 ± 18	420 ± 360	274 ± 30
43	474 ± 12	900 ± 120	400 ± 30
44	1170 ± 6	1218 ± 48	400 ± 30
45	623 ± 4	960 ± 60	270 ± 30
46	150 ± 5	216 ± 60	188 ± 20
47	122 ± 6	348 ± 360	160 ± 20
48	273 ± 54	468 ± 36	171 ± 20
49	282 ± 6	606 ± 186	122 ± 20
50	491 ± 18	834 ± 6	262 ± 20
51	348 ± 7	906 ± 288	238 ± 20
52	340 ± 3	930 ± 144	200 ± 20

Notes.

⁽¹⁾

The reference citations are listed in Fig. 1.

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