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| 20250723 - Filament data for 08 UTC |
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Available data for 20250723: »06 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1321 1594 (N39W29 L=301) 759 181 0 (1258/1541-1395/1630) 18.4 W22-W37 N35-N41
2 609 1569 (N43E31 L=241) 310 83 0 ( 568/1550- 657/1587) 7.1 E34-E26 N41-N44
3 964 1558 (N40E00 L=272) 668 217 3 ( 868/1530-1071/1583) -15.9 E07-W08 N37-N42
4 1063 1269 (N20W04 L=276) 212 65 1 (1032/1253-1096/1288) -26.6 W02-W06 N18-N20
5 1584 1196 (N11W38 L=310) 786 243 2 (1498/1108-1645/1252) -45.0 W32-W42 N04-N14
6 523 1018 (N07E32 L=240) 862 370 0 ( 412/ 871- 629/1130) -46.8 E40-E25 S02-N14
7 928 1079 (N09E06 L=266) 207 85 0 ( 916/1030- 942/1115) 68.2 E06-E04 N06-N11
8 1907 1029 (S04W69 L=341) 764 59 0 (1879/1000-1933/1064) 38.7 W64-W74 S05-S01
9 1270 788 (S11W14 L=286) 225 103 1 (1252/ 740-1291/ 832) 80.5 W12-W15 S14-S08
10 297 673 (S14E57 L=215) 1783 306 3 ( 238/ 606- 360/ 761) -58.0 E63-E51 S18-S08
11 915 658 (S17E10 L=262) 221 123 0 ( 891/ 623- 932/ 706) -80.5 E11-E08 S19-S13
12 1747 637 (S27W53 L=325) 921 125 1 (1694/ 595-1801/ 674) 15.3 W48-W59 S28-S24
13 1113 583 (S23W03 L=275) 496 215 0 (1036/ 530-1191/ 655) 35.0 E02-W08 S26-S19
14 239 613 (S18E68 L=204) 654 58 3 ( 222/ 579- 254/ 640) 53.1 E71-E64 S20-S16
15 676 547 (S23E27 L=244) 733 308 1 ( 619/ 423- 742/ 639) 53.7 E34-E21 S31-S16
16 1595 507 (S34W41 L=313) 324 35 1 (1580/ 486-1619/ 531) -56.3 W38-W43 S35-S32
17 1520 383 (S43W38 L=310) 3010 394 10 (1342/ 332-1644/ 465) -1.7 W20-W53 S48-S36
18 1186 316 (S45W07 L=279) 323 47 1 (1164/ 294-1211/ 346) 63.4 W05-W09 S46-S42
19 885 251 (S48E21 L=251) 3177 541 8 ( 664/ 188-1095/ 317) 4.9 E50-W00 S54-S43
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Download FITS filament maps as tar archive
» All Filament Data of 20250723 ...
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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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