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| 20240910 - Filament data for 11 UTC |
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Available data for 20240910: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1155 1755 (N47W39 L=159) 353 61 0 (1139/1722-1169/1793) 35.5 W35-W42 N44-N49
2 1410 1592 (N28W44 L=164) 1185 230 2 (1315/1523-1501/1639) 0.0 W33-W53 N26-N30
3 1517 1433 (N16W42 L=162) 494 158 2 (1451/1393-1578/1476) 4.8 W36-W48 N15-N17
4 1091 1364 (N25W13 L=133) 696 160 3 (1031/1318-1166/1399) 0.0 W08-W17 N22-N26
5 1790 1037 (S13W50 L=170) 4954 955 10 (1598/ 838-1900/1279) 21.0 W31-W70 S20-S03
6 807 1245 (N25E08 L=113) 213 52 1 ( 782/1222- 832/1268) 14.0 E09-E05 N23-N25
7 1076 1175 (N14W07 L=127) 241 119 0 (1039/1125-1104/1221) -81.9 W05-W07 N10-N17
8 793 1146 (N19E11 L=110) 216 72 0 ( 754/1126- 821/1162) -45.0 E12-E09 N17-N20
9 1201 1115 (N08W12 L=132) 244 108 0 (1172/1066-1240/1156) 33.7 W09-W15 N05-N09
10 860 1043 (N12E09 L=111) 209 81 0 ( 817/1029- 897/1061) -31.0 E11-E06 N10-N14
11 571 982 (N15E28 L= 92) 390 62 3 ( 539/ 952- 600/1016) -45.0 E30-E26 N12-N16
12 868 767 (S04E15 L=105) 487 198 1 ( 801/ 717- 958/ 809) -53.1 E17-E11 S08-N00
13 1515 744 (S22W23 L=143) 229 55 0 (1502/ 711-1527/ 778) 76.0 W21-W23 S23-S19
14 1817 744 (S32W51 L=171) 642 111 0 (1766/ 719-1858/ 776) -4.8 W44-W56 S33-S30
15 1525 554 (S35W21 L=141) 1364 386 0 (1394/ 436-1629/ 709) 28.6 W08-W30 S39-S27
16 1201 580 (S23E01 L=119) 461 206 1 (1129/ 522-1264/ 665) 26.6 E06-W05 S24-S19
17 1675 486 (S47W36 L=157) 937 129 1 (1628/ 451-1715/ 535) 0.0 W30-W40 S49-S42
18 1011 428 (S28E17 L=103) 338 109 0 ( 982/ 408-1057/ 473) -59.0 E18-E14 S29-S24
19 445 401 (S18E59 L= 61) 420 54 0 ( 433/ 366- 456/ 431) 51.3 E61-E56 S20-S15
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Download FITS filament maps as tar archive
» All Filament Data of 20240910 ...
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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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