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| 20231229 - Filament data for 12 UTC |
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Available data for 20231229: »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 1220 1781 (N49W21 L=282) 1356 178 5 (1154/1731-1303/1840) -36.0 W16-W27 N43-N54
2 1615 1661 (N38W55 L=315) 1297 194 1 (1516/1638-1698/1682) 0.0 W44-W72 N36-N39
3 1541 1482 (N25W38 L=298) 7963 1115 13 (1113/1178-1901/1649) -20.7 W07-W69 N05-N37
4 1531 1363 (N17W35 L=295) 420 106 1 (1515/1308-1553/1414) -90.0 W33-W36 N13-N20
5 824 1348 (N18E12 L=248) 557 120 3 ( 774/1306- 876/1385) -45.0 E14-E08 N14-N20
6 1307 1291 (N13W18 L=278) 291 77 0 (1271/1252-1347/1322) -45.0 W16-W20 N10-N14
7 1747 1250 (N10W51 L=311) 429 75 2 (1734/1203-1774/1291) 80.5 W49-W53 N06-N12
8 1660 1257 (N10W43 L=303) 324 50 0 (1636/1234-1681/1287) 36.9 W41-W45 N08-N12
9 411 1206 (N11E40 L=220) 385 145 0 ( 359/1179- 474/1242) 20.6 E43-E35 N09-N12
10 978 1193 (N08E02 L=258) 271 81 0 ( 943/1160-1012/1227) -45.0 E04-W00 N05-N09
11 1894 873 (S13W67 L=327) 3507 279 2 (1845/ 764-1952/1018) 55.5 W62-W75 S19-S03
12 1606 788 (S18W39 L=299) 995 321 0 (1551/ 648-1678/ 922) 76.8 W35-W43 S26-S09
13 411 768 (S16E42 L=218) 822 215 3 ( 313/ 736- 502/ 791) 0.0 E50-E34 S17-S13
14 397 602 (S26E48 L=212) 531 90 1 ( 366/ 571- 439/ 639) 24.0 E52-E43 S27-S23
15 1272 589 (S30W16 L=276) 242 84 0 (1245/ 553-1308/ 621) 45.0 W14-W18 S32-S28
16 1736 506 (S36W63 L=323) 1671 205 0 (1648/ 472-1808/ 559) 15.5 W50-W73 S38-S32
17 1472 465 (S39W34 L=295) 653 97 2 (1424/ 425-1511/ 505) -18.4 W29-W38 S42-S36
18 1156 449 (S40W08 L=268) 832 172 0 (1073/ 420-1244/ 486) 13.0 W01-W14 S41-S37
19 373 383 (S40E69 L=191) 832 75 1 ( 338/ 353- 402/ 418) 7.1 E83-E59 S42-S38
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Download FITS filament maps as tar archive
» All Filament Data of 20231229 ...
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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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