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| 20241230 - Filament data for 09 UTC |
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Available data for 20241230: »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 1383 1562 (N30W27 L=125) 2238 589 4 (1161/1464-1632/1681) -26.6 W12-W44 N23-N39
2 455 1515 (N30E40 L= 57) 824 136 4 ( 400/1449- 498/1563) -41.6 E47-E35 N25-N33
3 1199 1451 (N23W12 L=110) 555 157 1 (1163/1378-1218/1519) 71.6 W09-W13 N18-N27
4 1080 1463 (N24W05 L=103) 342 102 0 (1031/1441-1128/1482) 0.0 W01-W07 N22-N25
5 1308 1296 (N13W18 L=116) 497 198 0 (1292/1197-1325/1389) 80.5 W16-W19 N06-N18
6 1861 1293 (N13W63 L=161) 592 47 1 (1838/1263-1883/1322) -63.4 W60-W66 N10-N14
7 187 764 (S15E65 L= 33) 4837 584 10 ( 111/ 500- 252/1034) 81.1 E77-E60 S31-N01
8 747 960 (S06E17 L= 81) 281 54 2 ( 718/ 928- 772/ 992) 63.4 E18-E15 S07-S03
9 1872 874 (S13W62 L=160) 4847 354 13 (1767/ 731-1962/ 989) 37.3 W53-W75 S21-S05
10 800 915 (S09E14 L= 84) 418 85 1 ( 773/ 873- 824/ 950) -68.2 E15-E12 S11-S06
11 297 823 (S12E51 L= 47) 1084 164 3 ( 247/ 746- 354/ 861) 49.4 E55-E45 S16-S09
12 495 687 (S21E37 L= 61) 1908 520 4 ( 340/ 626- 629/ 825) 0.0 E49-E26 S24-S13
13 1895 777 (S18W69 L=166) 988 90 4 (1875/ 725-1921/ 822) 80.5 W65-W72 S21-S15
14 1554 612 (S29W37 L=135) 247 82 1 (1538/ 584-1578/ 660) -68.2 W35-W39 S30-S25
15 1216 555 (S32W12 L=110) 228 80 0 (1175/ 542-1257/ 568) -11.3 W09-W14 S33-S31
16 881 409 (S42E14 L= 84) 1022 248 2 ( 781/ 346- 991/ 486) 25.3 E23-E04 S46-S36
17 680 299 (S49E36 L= 61) 335 52 1 ( 648/ 279- 706/ 314) 0.0 E40-E33 S50-S47
18 1256 208 (S61W24 L=122) 611 34 1 (1231/ 186-1281/ 235) -33.7 W20-W29 S63-S57
19 1190 205 (S61W16 L=114) 727 100 1 (1154/ 179-1231/ 230) -24.4 W10-W21 S63-S58
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Download FITS filament maps as tar archive
» All Filament Data of 20241230 ...
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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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