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| 20250702 - Filament data for 08 UTC |
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Available data for 20250702: »05 UTC »06 UTC »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
1 763 1759 (N53E31 L=159) 449 80 2 ( 716/1739- 799/1777) 7.1 E35-E27 N51-N54
2 1587 1679 (N48W58 L=248) 610 53 0 (1552/1658-1617/1698) 7.6 W50-W65 N45-N49
3 1188 1547 (N37W11 L=201) 417 94 0 (1144/1525-1231/1568) 8.1 W07-W14 N35-N38
4 305 1524 (N31E67 L=123) 698 88 1 ( 273/1507- 347/1546) -6.7 E76-E59 N30-N32
5 1246 1491 (N33W15 L=205) 272 43 1 (1224/1470-1266/1522) 76.0 W13-W16 N31-N35
6 460 1475 (N29E45 L=145) 1128 214 3 ( 390/1440- 562/1508) -6.7 E52-E35 N26-N31
7 1265 1325 (N22W15 L=205) 404 106 2 (1245/1269-1287/1373) 66.8 W13-W16 N18-N25
8 285 1168 (N09E53 L=137) 810 176 0 ( 261/1096- 316/1256) -51.3 E57-E49 N04-N14
9 1676 1048 (N05W44 L=234) 1512 335 0 (1590/ 919-1720/1181) -59.0 W37-W47 S02-N13
10 591 1066 (N04E28 L=163) 230 48 0 ( 574/1037- 613/1090) 71.6 E28-E26 N02-N05
11 1843 808 (S10W63 L=253) 873 109 2 (1816/ 755-1867/ 865) -74.1 W60-W66 S13-S06
12 1580 752 (S13W38 L=228) 313 57 1 (1561/ 728-1597/ 780) -56.3 W36-W39 S14-S11
13 265 698 (S21E58 L=132) 769 140 0 ( 212/ 660- 308/ 738) 20.6 E67-E51 S23-S17
14 588 635 (S23E29 L=161) 243 107 0 ( 575/ 584- 608/ 683) 74.1 E30-E27 S26-S19
15 1763 588 (S24W62 L=252) 2850 203 5 (1683/ 523-1817/ 663) 48.4 W54-W69 S28-S19
16 870 578 (S26E09 L=181) 831 182 0 ( 802/ 545- 953/ 635) -21.8 E13-E03 S27-S21
17 659 584 (S26E24 L=166) 403 123 0 ( 601/ 562- 710/ 620) 20.6 E28-E20 S27-S23
18 1284 218 (S55W33 L=223) 2626 218 8 (1186/ 183-1401/ 252) 11.3 W21-W49 S59-S51
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Download FITS filament maps as tar archive
» All Filament Data of 20250702 ...
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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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