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| 20230220 - Filament data for 10 UTC |
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Available data for 20230220: »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 1071 1806 (N45E19 L= 42) 499 61 1 (1047/1776-1093/1837) -33.7 E22-E16 N42-N48
2 1161 1627 (N33E05 L= 55) 422 95 1 (1117/1602-1216/1657) 0.0 E08-E01 N31-N34
3 1360 1527 (N31W10 L= 71) 948 182 3 (1314/1463-1424/1595) -31.0 W05-W15 N28-N34
4 1637 1504 (N38W33 L= 94) 1307 133 3 (1592/1446-1668/1569) -83.7 W28-W36 N33-N42
5 478 1297 (S01E39 L= 22) 382 48 0 ( 451/1270- 508/1324) 33.7 E41-E37 S02-N00
6 1678 1090 (N12W39 L=100) 1840 500 5 (1635/ 858-1714/1286) -66.5 W33-W45 S01-N22
7 424 1222 (S06E42 L= 19) 340 42 0 ( 396/1200- 451/1247) -21.8 E44-E39 S07-S04
8 1828 1170 (N21W53 L=113) 549 75 2 (1801/1148-1859/1205) -9.5 W49-W56 N19-N22
9 1871 1037 (N15W59 L=120) 1836 242 5 (1828/ 920-1895/1136) -85.9 W54-W64 N07-N21
10 1809 1076 (N15W51 L=112) 315 51 1 (1789/1049-1826/1103) -33.7 W48-W53 N13-N16
11 268 947 (S25E52 L= 9) 456 90 1 ( 252/ 901- 282/ 985) 90.0 E53-E50 S27-S22
12 383 653 (S42E42 L= 19) 363 84 0 ( 352/ 620- 424/ 680) 29.1 E46-E37 S44-S39
13 1715 645 (S11W56 L=117) 559 76 1 (1687/ 603-1742/ 672) 68.2 W53-W58 S14-S09
14 1196 620 (S26W20 L= 81) 320 96 0 (1153/ 589-1241/ 649) -7.1 W16-W24 S27-S25
15 1420 537 (S25W38 L= 99) 929 179 3 (1351/ 478-1484/ 595) -12.1 W32-W46 S27-S23
16 1339 404 (S35W40 L=101) 719 141 1 (1275/ 376-1410/ 441) 4.1 W33-W47 S36-S34
17 1266 331 (S42W41 L=101) 441 76 1 (1246/ 296-1296/ 365) -12.5 W36-W45 S44-S39
18 1554 311 (S34W69 L=130) 821 94 2 (1504/ 295-1603/ 335) 35.5 W63-W73 S36-S31
19 1358 241 (S45W59 L=119) 811 63 0 (1334/ 204-1381/ 283) -22.6 W52-W65 S47-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20230220 ...
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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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