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| 20250101 - Filament data for 08 UTC |
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Available data for 20250101: »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 1043 1752 (N46W03 L= 75) 401 32 0 (1012/1734-1073/1772) 0.0 W00-W05 N43-N47
2 1077 1678 (N39W05 L= 77) 373 62 1 (1059/1648-1105/1716) 71.6 W03-W07 N36-N42
3 1648 1562 (N31W50 L=122) 1508 202 1 (1566/1517-1738/1618) -28.3 W43-W58 N27-N34
4 779 1573 (N32E16 L= 56) 716 143 0 ( 712/1525- 834/1601) -29.1 E21-E12 N28-N34
5 1763 1501 (N27W60 L=132) 637 54 1 (1736/1475-1791/1530) 24.0 W55-W65 N24-N28
6 1419 1471 (N24W27 L= 99) 703 159 1 (1348/1434-1511/1495) 0.0 W22-W34 N21-N25
7 1595 1429 (N21W40 L=112) 660 122 0 (1565/1374-1620/1475) 74.1 W37-W42 N17-N24
8 1846 1276 (N12W61 L=133) 3112 254 6 (1793/1167-1926/1381) -47.7 W53-W72 N05-N18
9 1680 1245 (N10W44 L=116) 658 182 1 (1655/1153-1708/1330) -79.7 W42-W45 N04-N15
10 407 725 (S19E43 L= 29) 4946 875 8 ( 303/ 375- 464/1087) 42.4 E89-E36 S40-N02
11 230 1025 (S00E55 L= 17) 557 188 0 ( 182/ 961- 267/1074) -45.0 E60-E51 S04-N02
12 190 852 (S10E62 L= 10) 5178 311 11 ( 123/ 707- 280/ 999) 73.6 E71-E52 S18-S01
13 612 891 (S10E26 L= 46) 319 48 1 ( 573/ 870- 645/ 917) 0.0 E28-E23 S11-S08
14 917 720 (S21E07 L= 65) 1485 487 1 ( 733/ 653-1016/ 873) 21.3 E19-W00 S25-S11
15 1182 822 (S15W09 L= 81) 585 261 2 (1124/ 739-1261/ 862) 45.0 W05-W14 S20-S12
16 289 753 (S17E53 L= 19) 659 91 0 ( 257/ 709- 318/ 796) -51.3 E55-E51 S19-S14
17 233 762 (S16E59 L= 13) 593 57 2 ( 200/ 731- 261/ 783) -36.9 E62-E55 S17-S14
18 1329 481 (S38W22 L= 94) 2528 594 6 (1088/ 372-1605/ 570) 16.7 W03-W43 S45-S31
19 1174 250 (S56W14 L= 86) 394 73 1 (1131/ 233-1199/ 278) 33.7 W09-W17 S58-S53
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Download FITS filament maps as tar archive
» All Filament Data of 20250101 ...
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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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