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| 20260703 - Filament data for 11 UTC |
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Available data for 20260703: »06 UTC »07 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
1 640 1297 (N19E26 L= 11) 334 71 0 ( 623/1268- 664/1336) -53.1 E27-E24 N16-N20
2 1785 1264 (N19W57 L= 95) 485 55 1 (1762/1235-1804/1299) 53.1 W54-W60 N16-N20
3 1733 1268 (N19W51 L= 89) 340 31 0 (1717/1247-1749/1296) -71.6 W49-W53 N17-N20
4 993 1239 (N16E03 L= 35) 288 99 0 ( 956/1206-1036/1275) -38.7 E05-W00 N14-N18
5 819 1179 (N12E13 L= 24) 499 167 0 ( 798/1103- 846/1254) 77.5 E14-E12 N07-N16
6 1708 1226 (N16W48 L= 86) 343 50 0 (1679/1209-1738/1244) -11.3 W45-W51 N15-N17
7 1616 1174 (N13W40 L= 77) 308 55 0 (1591/1146-1640/1201) -45.0 W37-W41 N11-N14
8 1278 1114 (N09W16 L= 53) 502 193 0 (1195/1057-1340/1158) -33.7 W10-W19 N05-N11
9 243 835 (S12E57 L=341) 1366 223 3 ( 192/ 741- 278/ 946) -72.9 E62-E53 S18-S05
10 1547 883 (S05W34 L= 72) 473 72 0 (1516/ 851-1580/ 911) 36.9 W32-W36 S06-S02
11 1597 838 (S07W38 L= 76) 643 107 2 (1557/ 788-1641/ 886) 63.4 W35-W41 S10-S04
12 1749 813 (S09W52 L= 90) 1120 210 2 (1681/ 773-1816/ 858) -8.1 W45-W59 S11-S06
13 1819 731 (S14W62 L=100) 1878 180 9 (1764/ 653-1864/ 809) 73.3 W57-W67 S19-S09
14 777 669 (S20E15 L= 23) 728 200 0 ( 715/ 591- 828/ 746) 54.0 E19-E11 S25-S14
15 1740 693 (S17W54 L= 92) 355 54 0 (1722/ 668-1758/ 719) -71.6 W52-W56 S18-S15
16 599 520 (S31E30 L= 8) 609 105 0 ( 532/ 497- 650/ 548) 10.3 E36-E25 S33-S28
17 1589 511 (S29W46 L= 83) 377 85 0 (1545/ 486-1622/ 544) 38.7 W42-W48 S30-S26
18 1587 424 (S36W51 L= 88) 1214 138 1 (1528/ 375-1643/ 476) 36.9 W46-W55 S39-S31
19 762 254 (S53E24 L= 14) 539 76 0 ( 723/ 240- 799/ 273) 15.3 E29-E18 S55-S51
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Download FITS filament maps as tar archive
» All Filament Data of 20260703 ...
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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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