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| 20231027 - Filament data for 11 UTC |
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Available data for 20231027: »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 1426 1788 (N36W63 L= 74) 462 49 0 (1394/1766-1451/1805) -5.2 W56-W67 N35-N37
2 1427 1707 (N32W53 L= 64) 350 74 1 (1391/1688-1459/1732) -68.2 W51-W55 N29-N34
3 593 1613 (N53E15 L=356) 2208 410 5 ( 413/1522- 757/1686) -3.0 E37-W01 N50-N56
4 1120 1434 (N25W17 L= 28) 437 100 1 (1084/1385-1144/1478) 81.9 W15-W18 N21-N28
5 440 1325 (N37E32 L=338) 534 114 2 ( 389/1272- 476/1358) -49.4 E37-E28 N33-N40
6 1176 1254 (N14W15 L= 26) 496 114 3 (1134/1227-1229/1290) -51.3 W12-W17 N11-N16
7 195 1040 (N25E60 L=311) 991 159 0 ( 143/ 983- 258/1088) -31.6 E68-E53 N20-N28
8 658 1008 (N13E21 L=350) 262 65 2 ( 630/ 990- 696/1029) 0.0 E23-E18 N11-N14
9 1892 990 (S22W62 L= 73) 678 94 1 (1851/ 967-1929/1017) -24.4 W56-W68 S24-S18
10 171 859 (N14E67 L=304) 3199 374 3 ( 110/ 698- 234/1005) -67.2 E75-E61 N04-N23
11 295 955 (N18E50 L=321) 523 112 0 ( 268/ 906- 328/1001) -80.5 E52-E47 N14-N20
12 246 856 (N13E57 L=314) 641 69 1 ( 222/ 826- 277/ 889) -76.0 E59-E53 N11-N15
13 1123 727 (S14E02 L= 9) 904 336 0 (1036/ 586-1213/ 860) 38.7 E10-W06 S20-S08
14 1344 663 (S24W09 L= 20) 877 195 2 (1261/ 599-1401/ 745) 24.4 W02-W14 S26-S20
15 1604 643 (S34W28 L= 39) 345 55 1 (1569/ 620-1632/ 662) -31.0 W25-W30 S35-S31
16 873 610 (S15E20 L=351) 285 98 0 ( 833/ 583- 919/ 642) -63.4 E21-E17 S17-S11
17 437 506 (S11E54 L=317) 558 162 0 ( 381/ 468- 501/ 547) -45.0 E57-E50 S14-S07
18 1536 520 (S40W21 L= 32) 269 38 1 (1515/ 499-1556/ 541) -45.0 W19-W22 S41-S38
19 570 292 (S28E59 L=312) 753 98 1 ( 547/ 241- 602/ 328) 21.8 E67-E52 S31-S25
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Download FITS filament maps as tar archive
» All Filament Data of 20231027 ...
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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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