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| 20241025 - Filament data for 10 UTC |
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Available data for 20241025: »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 1563 1741 (N28W69 L=316) 824 62 1 (1530/1706-1587/1769) -4.8 W63-W75 N25-N29
2 979 1604 (N39W16 L=263) 389 147 0 ( 898/1588-1042/1618) -15.3 W09-W20 N36-N41
3 1722 1513 (N11W63 L=310) 2009 314 2 (1592/1416-1833/1582) -43.2 W53-W70 N02-N17
4 330 1362 (N42E43 L=204) 302 50 1 ( 308/1344- 353/1379) -26.6 E46-E40 N40-N43
5 1411 1326 (N11W30 L=278) 213 54 2 (1393/1299-1431/1350) -90.0 W28-W31 N09-N12
6 712 1232 (N24E13 L=234) 227 96 1 ( 673/1212- 763/1252) -18.4 E15-E09 N22-N25
7 1296 1170 (N06W19 L=266) 453 108 1 (1238/1148-1354/1185) -33.7 W15-W21 N03-N07
8 1119 1048 (N04W06 L=253) 716 237 1 (1028/ 995-1197/1148) 18.4 W00-W12 N01-N07
9 796 1090 (N14E11 L=236) 239 70 0 ( 762/1073- 840/1108) 0.0 E13-E08 N13-N15
10 1813 942 (S22W50 L=297) 1174 148 3 (1768/ 869-1866/ 997) 20.0 W45-W56 S25-S18
11 550 898 (N09E31 L=217) 721 164 1 ( 493/ 839- 595/ 972) 21.8 E35-E25 N05-N12
12 278 929 (N17E51 L=196) 301 48 2 ( 253/ 914- 312/ 949) -9.5 E53-E47 N15-N18
13 1222 858 (S09W07 L=254) 184 74 0 (1197/ 831-1244/ 899) -90.0 W05-W07 S11-S06
14 1669 748 (S29W34 L=281) 661 111 1 (1622/ 707-1719/ 786) 6.3 W29-W38 S30-S27
15 403 484 (S11E57 L=190) 8808 0 24 ( 229/ 289- 581/ 754) -79.0 E72-E46 S25-N07
16 550 590 (S08E40 L=207) 268 30 1 ( 529/ 566- 573/ 608) 41.8 E41-E37 S09-S06
17 920 528 (S20E20 L=228) 516 179 0 ( 894/ 444- 950/ 603) 41.6 E24-E15 S24-S16
18 651 534 (S13E36 L=212) 628 108 3 ( 609/ 494- 699/ 582) -90.0 E39-E32 S16-S10
19 1483 533 (S37W16 L=263) 712 112 2 (1450/ 484-1526/ 569) 23.2 W12-W19 S39-S33
20 606 465 (S16E42 L=205) 1205 266 3 ( 483/ 410- 695/ 541) -42.3 E47-E36 S20-S09
21 650 244 (S32E55 L=192) 1520 213 2 ( 587/ 194- 688/ 316) 39.8 E64-E48 S36-S26
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Download FITS filament maps as tar archive
» All Filament Data of 20241025 ...
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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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