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| 20251111 - Filament data for 11 UTC |
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Available data for 20251111: »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 1456 1678 (N30W50 L=295) 560 113 0 (1417/1628-1491/1710) 80.5 W47-W52 N26-N32
2 1209 1579 (N31W27 L=272) 245 82 1 (1188/1540-1232/1614) 59.0 W24-W28 N28-N33
3 541 1560 (N47E23 L=222) 388 55 1 ( 514/1537- 578/1578) -9.5 E25-E19 N45-N49
4 1421 1548 (N23W39 L=284) 424 80 1 (1387/1524-1463/1573) -53.1 W36-W41 N21-N25
5 401 1528 (N49E39 L=206) 620 79 1 ( 373/1487- 432/1564) 68.2 E42-E34 N45-N51
6 1431 1432 (N17W35 L=280) 472 206 0 (1349/1385-1494/1496) 8.7 W27-W40 N15-N19
7 919 1468 (N31W04 L=249) 1063 273 2 ( 783/1442-1045/1487) -14.0 E04-W12 N28-N33
8 1209 1196 (N09W14 L=259) 1246 327 2 (1082/1153-1366/1233) -13.2 W06-W23 N04-N11
9 1808 1129 (S09W54 L=299) 309 40 1 (1787/1099-1822/1159) 56.3 W51-W55 S11-S07
10 350 1009 (N16E43 L=202) 1005 200 4 ( 268/ 934- 428/1065) -36.9 E50-E37 N10-N20
11 572 822 (N01E31 L=214) 214 71 0 ( 556/ 786- 586/ 862) 71.6 E32-E29 N00-N03
12 1079 806 (S10E02 L=243) 184 69 1 (1058/ 764-1093/ 836) 76.0 E02-W00 S12-S08
13 1060 668 (S18E06 L=239) 276 98 1 (1020/ 639-1098/ 702) -59.0 E07-E04 S20-S14
14 1669 658 (S34W36 L=281) 685 143 1 (1603/ 623-1722/ 700) 5.2 W29-W40 S35-S31
15 645 607 (S12E32 L=213) 285 109 0 ( 586/ 590- 693/ 628) -7.1 E36-E28 S13-S10
16 533 585 (S11E41 L=204) 254 71 1 ( 519/ 553- 550/ 616) 53.1 E42-E38 S13-S09
17 649 490 (S19E37 L=208) 235 51 1 ( 636/ 458- 662/ 521) 53.1 E38-E34 S21-S17
18 547 332 (S27E54 L=191) 1787 224 3 ( 459/ 287- 665/ 364) 0.0 E69-E42 S29-S24
19 987 242 (S45E28 L=217) 1402 188 2 ( 902/ 198-1064/ 299) 6.7 E36-E19 S47-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20251111 ...
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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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