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| 20251028 - Filament data for 07 UTC |
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Available data for 20251028: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 646 1751 (N63E07 L= 65) 389 40 1 ( 623/1726- 671/1772) 0.0 E09-E02 N60-N64
2 1488 1678 (N28W54 L=126) 932 189 0 (1423/1600-1534/1741) 63.4 W49-W57 N23-N33
3 1570 1601 (N21W55 L=126) 439 40 0 (1544/1583-1603/1617) -36.9 W51-W58 N19-N22
4 1279 1495 (N24W29 L=100) 223 45 1 (1248/1479-1306/1508) -33.7 W27-W30 N22-N25
5 1045 1394 (N25W11 L= 83) 1268 208 3 ( 950/1331-1143/1426) -35.0 W05-W17 N21-N28
6 1367 1182 (N05W23 L= 95) 412 165 0 (1302/1158-1418/1229) -7.1 W19-W27 N03-N07
7 1858 1075 (S15W58 L=129) 1065 210 3 (1829/ 977-1891/1156) 42.0 W52-W63 S20-S11
8 1732 1073 (S11W45 L=116) 269 57 0 (1704/1051-1759/1101) -53.1 W43-W46 S13-S09
9 646 1025 (N14E22 L= 50) 206 75 0 ( 603/1008- 681/1043) -11.3 E24-E19 N12-N14
10 900 963 (N04E08 L= 63) 271 26 0 ( 876/ 940- 921/ 986) 26.6 E10-E06 N03-N05
11 1822 759 (S33W51 L=122) 1131 222 3 (1771/ 663-1876/ 859) 45.0 W44-W57 S38-S28
12 681 715 (S04E27 L= 44) 1214 352 0 ( 537/ 628- 785/ 827) 15.9 E39-E18 S06-N00
13 203 719 (N05E66 L= 5) 559 48 1 ( 176/ 694- 231/ 745) -31.0 E69-E63 N03-N07
14 1656 567 (S41W32 L=104) 329 51 0 (1643/ 540-1671/ 598) -63.4 W31-W34 S42-S38
15 349 512 (S09E60 L= 11) 503 77 1 ( 330/ 478- 368/ 543) 14.0 E65-E57 S11-S07
16 1464 458 (S42W14 L= 85) 357 86 0 (1429/ 435-1495/ 490) 18.4 W10-W16 S43-S40
17 410 415 (S16E61 L= 10) 993 150 1 ( 368/ 378- 436/ 476) 26.6 E67-E55 S18-S12
18 1396 410 (S43W07 L= 79) 269 31 1 (1382/ 391-1416/ 434) 71.6 W05-W09 S44-S40
19 1003 244 (S43E29 L= 43) 725 114 2 ( 942/ 224-1063/ 270) -5.2 E34-E23 S44-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20251028 ...
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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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