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| 20240727 - Filament data for 11 UTC |
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Available data for 20240727: »05 UTC »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
1 511 1394 (N33E35 L=320) 911 255 1 ( 424/1308- 593/1444) -30.5 E44-E27 N26-N36
2 1155 1247 (N18W10 L= 6) 203 52 0 (1141/1215-1166/1279) -90.0 W09-W11 N15-N19
3 179 1219 (N22E68 L=287) 732 94 3 ( 163/1168- 191/1263) -63.4 E72-E65 N19-N25
4 1729 1057 (S01W48 L= 44) 975 200 0 (1711/ 966-1755/1147) 63.4 W46-W52 S06-N04
5 1692 862 (S13W44 L= 39) 375 87 0 (1655/ 835-1725/ 901) 26.6 W40-W46 S13-S10
6 674 868 (S01E23 L=332) 247 106 0 ( 629/ 834- 715/ 896) -31.0 E25-E20 S03-N00
7 1839 820 (S18W60 L= 55) 821 156 0 (1806/ 781-1867/ 860) 51.3 W56-W64 S20-S15
8 636 751 (S08E27 L=328) 427 65 1 ( 602/ 725- 676/ 773) 11.3 E29-E24 S09-S06
9 1260 678 (S19W12 L= 7) 389 161 0 (1234/ 631-1292/ 727) -63.4 W09-W13 S21-S15
10 553 679 (S12E34 L=321) 502 117 2 ( 527/ 628- 579/ 721) 71.6 E36-E31 S15-S09
11 733 651 (S15E22 L=333) 658 204 0 ( 655/ 618- 769/ 721) -15.9 E27-E19 S17-S10
12 219 660 (S13E69 L=286) 647 67 2 ( 193/ 627- 239/ 689) -63.4 E73-E66 S14-S10
13 1418 559 (S29W23 L= 18) 1585 402 2 (1288/ 462-1589/ 670) 23.5 W12-W35 S34-S23
14 943 642 (S17E09 L=346) 326 79 1 ( 902/ 627- 989/ 657) 0.0 E11-E05 S18-S16
15 1741 630 (S29W52 L= 47) 585 59 3 (1701/ 613-1779/ 652) -11.3 W47-W57 S30-S27
16 1001 552 (S24E07 L=349) 436 120 0 ( 975/ 505-1043/ 601) 50.2 E08-E03 S27-S21
17 1488 470 (S37W30 L= 25) 1107 261 1 (1370/ 430-1590/ 532) 9.0 W19-W38 S38-S33
18 1014 369 (S38E09 L=346) 378 74 1 ( 981/ 351-1059/ 386) 0.0 E11-E05 S39-S36
19 1086 307 (S45E04 L=351) 1777 235 4 (1015/ 229-1175/ 374) 42.7 E11-W03 S52-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20240727 ...
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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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