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| 20260210 - Filament data for 09 UTC |
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Available data for 20260210: »07 UTC »08 UTC »09 UTC »10 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 1170 1625 (N33E02 L=125) 572 92 1 (1128/1577-1203/1662) -38.7 E05-W00 N29-N35
2 284 1503 (N12E63 L= 64) 2830 267 9 ( 212/1417- 362/1608) 61.7 E69-E58 N06-N19
3 1339 1530 (N30W11 L=138) 1353 294 4 (1236/1438-1436/1596) -21.8 W03-W18 N24-N34
4 1383 1132 (N06W19 L=146) 897 187 2 (1287/1084-1465/1190) -9.5 W12-W24 N04-N07
5 121 1141 (S11E71 L= 56) 1094 100 3 ( 73/1111- 163/1180) 6.3 E82-E64 S12-S08
6 1946 1065 (N16W69 L=197) 2111 154 4 (1921/ 986-1972/1134) -63.4 W65-W76 N12-N20
7 1874 1078 (N14W58 L=186) 523 63 2 (1855/1053-1896/1120) -56.3 W55-W61 N12-N16
8 554 1019 (S14E29 L= 99) 349 125 0 ( 502/ 979- 599/1056) 45.0 E31-E25 S17-S11
9 1442 1015 (N01W25 L=152) 282 77 1 (1422/ 970-1466/1056) -56.3 W23-W25 S01-N02
10 1885 993 (N10W61 L=188) 400 64 0 (1858/ 971-1903/1026) 38.7 W57-W63 N07-N12
11 722 954 (S15E17 L=110) 410 133 2 ( 648/ 918- 777/ 987) 20.6 E21-E13 S17-S13
12 1599 816 (S07W39 L=167) 566 124 3 (1549/ 757-1643/ 849) -12.5 W35-W44 S09-S04
13 1273 772 (S16W19 L=147) 210 104 0 (1224/ 750-1322/ 805) 51.3 W16-W21 S18-S13
14 647 701 (S32E19 L=108) 1639 404 2 ( 474/ 627- 846/ 773) 25.7 E33-E05 S39-S24
15 1611 700 (S13W44 L=171) 247 81 0 (1576/ 675-1639/ 734) 68.2 W42-W45 S15-S10
16 1146 668 (S25W14 L=142) 280 145 0 (1116/ 625-1199/ 714) -9.5 W12-W18 S26-S21
17 353 578 (S44E48 L= 79) 688 83 1 ( 308/ 535- 392/ 611) 23.2 E56-E42 S47-S41
18 1675 569 (S19W55 L=183) 466 77 1 (1652/ 541-1704/ 607) -76.0 W52-W59 S20-S16
19 1311 443 (S35W34 L=161) 2048 402 4 (1145/ 324-1464/ 531) 57.0 W27-W40 S46-S26
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Data will be available after one hour of observations. |
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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