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| 20241015 - Filament data for 10 UTC |
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Available data for 20241015: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1620 1712 (N24W73 L= 92) 1666 132 2 (1565/1670-1681/1738) -18.4 W64-W82 N20-N26
2 1900 1251 (S09W70 L= 89) 957 103 4 (1871/1216-1929/1294) -68.2 W64-W74 S11-S06
3 314 1224 (N35E45 L=335) 778 178 0 ( 236/1162- 376/1262) -31.0 E54-E38 N29-N38
4 750 1055 (N14E15 L= 5) 219 62 0 ( 725/1033- 766/1084) 18.4 E16-E13 N13-N16
5 121 1051 (N28E71 L=308) 959 91 1 ( 73/1024- 163/1072) -2.5 E86-E63 N26-N29
6 706 1013 (N13E18 L= 1) 242 80 1 ( 675/ 978- 737/1034) -76.0 E20-E17 N10-N14
7 1778 949 (S20W46 L= 65) 396 58 0 (1755/ 924-1799/ 983) 36.9 W43-W48 S21-S18
8 1386 930 (S09W17 L= 37) 287 96 1 (1352/ 911-1434/ 963) -59.0 W15-W19 S11-S06
9 1595 864 (S19W29 L= 48) 221 81 0 (1562/ 837-1612/ 899) 26.6 W26-W30 S20-S17
10 1317 804 (S14W10 L= 29) 652 220 2 (1237/ 749-1356/ 891) 54.5 W05-W13 S16-S09
11 1480 807 (S19W20 L= 39) 461 96 3 (1453/ 756-1509/ 860) 81.9 W18-W21 S22-S15
12 1786 839 (S27W45 L= 64) 393 84 0 (1748/ 812-1828/ 859) 0.0 W41-W50 S28-S26
13 863 707 (S07E17 L= 2) 941 284 0 ( 823/ 579- 908/ 818) 42.5 E23-E11 S13-S02
14 400 538 (S06E54 L=325) 343 52 1 ( 381/ 509- 415/ 563) -90.0 E55-E52 S08-S04
15 627 375 (S21E46 L=333) 2611 414 2 ( 554/ 230- 767/ 519) 20.4 E64-E29 S30-S14
16 403 470 (S11E58 L=321) 1301 156 4 ( 351/ 425- 475/ 508) -9.5 E66-E52 S14-S07
17 509 446 (S14E50 L=329) 704 85 3 ( 485/ 404- 529/ 494) 39.8 E53-E47 S16-S11
18 1404 459 (S39W07 L= 26) 381 51 1 (1386/ 423-1423/ 493) 78.7 W05-W08 S41-S36
19 1291 320 (S46E06 L= 13) 1704 243 4 (1211/ 243-1378/ 383) 18.4 E15-W03 S50-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20241015 ...
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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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