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| 20230907 - Filament data for 10 UTC |
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Available data for 20230907: »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 1603 1678 (N28W70 L= 21) 1644 152 2 (1542/1620-1658/1722) -90.0 W63-W74 N23-N31
2 593 1546 (N50E20 L=291) 317 43 0 ( 566/1527- 616/1567) 18.4 E23-E17 N48-N51
3 1370 1523 (N27W37 L=348) 331 110 0 (1326/1475-1408/1556) -71.6 W35-W38 N23-N29
4 1506 1523 (N23W47 L=358) 327 67 2 (1483/1486-1532/1549) 26.6 W44-W50 N20-N23
5 1630 1508 (N18W56 L= 8) 1017 176 1 (1552/1460-1702/1544) -48.4 W51-W60 N13-N22
6 840 1453 (N37E01 L=310) 280 42 1 ( 819/1422- 860/1476) 76.0 E02-W00 N34-N38
7 1020 1254 (N20W05 L=317) 218 59 0 (1006/1215-1033/1284) 53.1 W03-W06 N18-N22
8 1755 1159 (S04W51 L= 3) 387 81 1 (1734/1118-1784/1189) 26.6 W48-W54 S06-S02
9 193 1078 (N26E63 L=248) 661 64 3 ( 162/1045- 219/1112) -35.5 E68-E59 N23-N28
10 276 1042 (N23E53 L=259) 1699 370 2 ( 173/ 935- 412/1106) 8.4 E66-E39 N17-N26
11 1562 990 (S08W32 L=343) 276 42 0 (1544/ 967-1581/1015) 18.4 W29-W33 S09-S06
12 1845 854 (S26W56 L= 7) 1843 185 2 (1781/ 792-1918/ 917) 6.0 W47-W68 S28-S22
13 1698 865 (S20W40 L=351) 805 231 1 (1580/ 832-1766/ 907) -14.0 W30-W46 S22-S15
14 1067 807 (S06E03 L=309) 419 144 2 (1024/ 736-1102/ 860) 45.0 E06-W00 S09-S03
15 1511 744 (S21W23 L=335) 290 117 0 (1469/ 712-1565/ 771) 8.1 W20-W27 S22-S20
16 501 707 (S01E40 L=271) 406 115 1 ( 487/ 650- 515/ 766) 56.3 E41-E37 S04-N02
17 1041 339 (S36E18 L=293) 3349 648 8 ( 891/ 135-1205/ 639) 32.6 E50-W01 S52-S19
18 1396 458 (S38W11 L=322) 356 39 0 (1376/ 428-1410/ 494) 78.7 W08-W12 S40-S35
19 572 363 (S24E51 L=260) 383 95 0 ( 524/ 348- 617/ 379) 0.0 E56-E46 S24-S23
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Download FITS filament maps as tar archive
» All Filament Data of 20230907 ...
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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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