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| 20240713 - Filament data for 08 UTC |
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Available data for 20240713: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1362 1643 (N43W33 L=215) 614 138 1 (1298/1617-1422/1673) -24.0 W27-W37 N41-N46
2 1646 1498 (N31W53 L=235) 516 92 1 (1606/1473-1694/1519) -14.0 W49-W57 N28-N32
3 1200 1484 (N33W15 L=197) 389 68 0 (1166/1460-1235/1510) -36.9 W12-W17 N31-N34
4 231 1312 (N22E64 L=118) 600 133 0 ( 201/1269- 278/1335) 33.7 E68-E58 N19-N23
5 506 1299 (N22E36 L=146) 551 148 0 ( 451/1257- 552/1323) 23.2 E39-E31 N19-N23
6 1215 1249 (N17W13 L=195) 285 121 0 (1179/1197-1247/1296) -71.6 W11-W14 N14-N20
7 360 1212 (N17E47 L=135) 348 63 2 ( 338/1187- 383/1242) -36.9 E48-E44 N15-N18
8 844 1056 (N07E11 L=171) 210 93 0 ( 803/1044- 896/1065) 0.0 E13-E07 N05-N07
9 1062 863 (S06W02 L=184) 692 195 1 ( 975/ 806-1131/ 923) -41.2 E03-W05 S09-S01
10 1530 772 (S14W33 L=215) 500 113 0 (1502/ 723-1549/ 831) 81.9 W30-W34 S16-S09
11 237 754 (S12E61 L=121) 933 157 2 ( 222/ 675- 268/ 816) 45.0 E66-E55 S17-S08
12 712 689 (S16E21 L=161) 1295 274 4 ( 589/ 635- 829/ 754) -7.1 E29-E13 S19-S11
13 1735 718 (S19W52 L=234) 510 116 1 (1699/ 681-1767/ 751) 59.0 W48-W55 S21-S16
14 1118 610 (S22W05 L=187) 1350 343 2 (1011/ 499-1250/ 715) 43.0 E02-W13 S29-S15
15 1528 609 (S25W34 L=216) 449 118 0 (1489/ 563-1570/ 653) 50.2 W32-W37 S27-S21
16 835 607 (S22E14 L=168) 252 53 0 ( 818/ 585- 854/ 636) -90.0 E15-E12 S23-S19
17 983 229 (S54E09 L=173) 487 47 2 ( 962/ 200-1003/ 256) -74.1 E10-E06 S57-S50
18 1099 206 (S57W04 L=186) 861 115 1 (1058/ 189-1157/ 234) -24.4 W00-W11 S59-S53
19 1203 188 (S61W17 L=199) 713 69 0 (1181/ 161-1223/ 223) -83.7 W14-W21 S64-S55
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Download FITS filament maps as tar archive
» All Filament Data of 20240713 ...
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The tar archive contains filament maps for all processed Hα images
with at least quality=1.
The maps contain the values 0 and 1, where 1 is the position of a detected filament.
The header in the FITS files is mostly taken from the corresponding Hα file,
so it should be compatible with standard solar software routines.
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