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| 20250206 - Filament data for 12 UTC |
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Available data for 20250206: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 950 1731 (N37E19 L=297) 678 129 1 ( 884/1705-1018/1758) -5.2 E24-E13 N35-N38
2 707 1636 (N26E32 L=284) 292 47 1 ( 687/1618- 737/1659) 0.0 E33-E29 N25-N28
3 426 1489 (N14E48 L=268) 418 72 0 ( 395/1460- 462/1508) 45.0 E49-E44 N11-N15
4 230 1385 (N06E63 L=253) 966 106 2 ( 198/1334- 264/1431) 80.5 E66-E60 N02-N08
5 1355 1344 (N18W15 L=331) 391 169 0 (1283/1327-1441/1366) 11.3 W10-W20 N16-N19
6 1682 1237 (N18W39 L=355) 2380 335 9 (1557/1130-1772/1344) -21.3 W28-W47 N11-N22
7 521 1281 (N02E35 L=281) 560 117 0 ( 494/1223- 546/1329) 90.0 E36-E33 S01-N04
8 1621 1159 (N12W35 L=351) 697 135 3 (1587/1103-1649/1218) 76.0 W32-W36 N07-N15
9 1370 1177 (N08W18 L=334) 293 61 1 (1348/1142-1395/1213) 78.7 W16-W19 N05-N10
10 1455 1151 (N08W24 L=339) 528 119 3 (1410/1104-1493/1200) -18.4 W20-W26 N04-N10
11 1422 1050 (N01W23 L=339) 211 65 0 (1384/1038-1459/1064) 21.8 W20-W25 N00-N02
12 460 855 (S24E34 L=281) 322 107 0 ( 441/ 803- 477/ 907) 74.1 E36-E33 S27-S20
13 1849 832 (S02W61 L= 17) 506 66 0 (1817/ 810-1880/ 853) 31.0 W57-W64 S03-N00
14 608 786 (S26E23 L=293) 1153 267 3 ( 489/ 726- 738/ 833) 21.3 E32-E14 S31-S22
15 1544 725 (S15W38 L=354) 239 61 1 (1521/ 700-1565/ 747) -14.0 W36-W40 S15-S13
16 1432 595 (S24W35 L=350) 3930 859 7 (1162/ 512-1749/ 736) 3.4 W14-W64 S29-S13
17 469 526 (S45E37 L=279) 806 187 1 ( 375/ 500- 552/ 554) -3.0 E47-E28 S46-S43
18 756 487 (S44E10 L=306) 877 276 2 ( 642/ 449- 902/ 521) 2.6 E20-W02 S45-S41
19 1077 413 (S43W17 L=333) 310 89 1 (1043/ 393-1128/ 438) -7.1 W13-W21 S43-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20250206 ...
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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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