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| 20231003 - Filament data for 10 UTC |
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Available data for 20231003: »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 1703 (N25W72 L= 40) 781 65 0 (1569/1677-1630/1719) -56.3 W68-W78 N23-N26
2 1087 1656 (N41W27 L=355) 253 75 1 (1053/1638-1127/1677) -18.4 W24-W31 N40-N42
3 1620 1603 (N20W62 L= 30) 388 40 3 (1601/1575-1640/1627) 18.4 W59-W65 N18-N20
4 1440 1571 (N24W45 L= 13) 630 185 1 (1367/1506-1491/1609) -77.5 W41-W48 N19-N28
5 1330 1485 (N23W33 L= 1) 800 268 0 (1219/1441-1425/1519) -33.7 W24-W37 N17-N26
6 1068 1380 (N25W13 L=341) 605 191 2 (1017/1300-1111/1461) -90.0 W11-W14 N19-N31
7 304 1432 (N50E52 L=276) 543 69 0 ( 280/1404- 332/1458) 31.0 E56-E47 N47-N51
8 535 1313 (N36E25 L=303) 1128 186 4 ( 455/1266- 635/1354) -29.7 E31-E17 N31-N40
9 1209 1235 (N13W16 L=344) 510 185 2 (1162/1172-1279/1292) -73.3 W14-W18 N07-N17
10 728 1207 (N24E13 L=315) 269 97 0 ( 693/1176- 768/1243) -56.3 E14-E10 N21-N27
11 1624 983 (S13W35 L= 3) 1075 277 0 (1562/ 869-1676/1107) 35.5 W27-W41 S17-S07
12 865 1013 (N10E09 L=319) 767 247 1 ( 794/ 928- 955/1103) -77.0 E11-E05 N03-N16
13 278 962 (N20E52 L=276) 1927 329 6 ( 213/ 862- 339/1084) 77.0 E59-E46 N14-N27
14 573 943 (N13E29 L=299) 298 70 1 ( 544/ 921- 605/ 967) -45.0 E30-E27 N11-N14
15 1433 724 (S22W16 L=344) 316 140 0 (1372/ 698-1488/ 765) -6.3 W11-W20 S22-S20
16 263 728 (N07E60 L=268) 408 71 0 ( 227/ 714- 298/ 744) 0.0 E65-E56 N06-N07
17 1631 706 (S30W30 L=358) 862 113 2 (1594/ 655-1679/ 743) 14.0 W26-W34 S32-S26
18 835 333 (S30E35 L=293) 598 102 1 ( 799/ 306- 878/ 367) 12.5 E38-E29 S31-S27
19 1084 300 (S40E21 L=307) 582 128 1 (1053/ 246-1106/ 363) 48.4 E26-E17 S43-S34
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Download FITS filament maps as tar archive
» All Filament Data of 20231003 ...
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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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