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| 20250221 - Filament data for 07 UTC |
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Available data for 20250221: »07 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
1 860 1770 (N36E31 L= 90) 834 143 5 ( 800/1720- 921/1802) -17.1 E37-E24 N33-N37
2 1041 1604 (N28E12 L=109) 345 105 2 (1007/1569-1095/1631) 51.3 E13-E09 N25-N30
3 1389 1574 (N35W12 L=133) 929 205 4 (1295/1517-1455/1605) -4.8 W04-W16 N32-N36
4 1097 1349 (N13E03 L=119) 226 103 0 (1068/1300-1130/1393) -45.0 E05-W00 N10-N15
5 478 1254 (S04E38 L= 83) 376 143 0 ( 440/1198- 496/1304) 81.9 E40-E36 S07-N00
6 1655 1178 (N16W36 L=157) 579 131 0 (1600/1135-1700/1223) -14.0 W31-W39 N14-N17
7 189 1159 (S13E62 L= 59) 574 68 3 ( 153/1132- 226/1184) 0.0 E67-E57 S14-S11
8 722 1070 (S10E18 L=103) 521 231 0 ( 626/1013- 800/1131) 41.6 E23-E14 S14-S05
9 1886 1071 (N17W60 L=181) 516 105 2 (1870/1025-1904/1128) 74.1 W57-W62 N13-N20
10 1714 949 (N05W45 L=166) 781 184 1 (1692/ 860-1730/1047) -71.6 W41-W47 N00-N09
11 194 998 (S22E60 L= 61) 821 117 0 ( 148/ 953- 242/1038) 22.6 E66-E54 S24-S19
12 1180 894 (S11W12 L=133) 247 85 0 (1153/ 853-1199/ 928) -53.1 W09-W12 S13-S09
13 1217 792 (S16W16 L=137) 237 75 1 (1192/ 756-1238/ 824) 78.7 W14-W17 S18-S13
14 919 767 (S24E01 L=120) 304 109 0 ( 875/ 748- 970/ 802) 0.0 E04-W02 S24-S22
15 1700 683 (S10W52 L=173) 1245 167 6 (1639/ 591-1749/ 763) -59.0 W46-W56 S15-S04
16 1756 641 (S10W60 L=181) 742 128 1 (1717/ 597-1795/ 695) 74.1 W56-W62 S13-S06
17 1832 642 (S08W69 L=190) 1107 88 3 (1804/ 597-1871/ 688) -68.2 W65-W75 S10-S05
18 1638 475 (S23W59 L=180) 1381 221 0 (1528/ 450-1728/ 514) 33.7 W50-W65 S27-S17
19 1472 310 (S37W59 L=180) 751 117 2 (1400/ 286-1517/ 345) 29.1 W53-W63 S39-S34
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Download FITS filament maps as tar archive
» All Filament Data of 20250221 ...
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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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