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| 20221005 - Filament data for 09 UTC |
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Available data for 20221005: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1109 1763 (N47W38 L=117) 329 72 0 (1083/1748-1145/1784) -63.4 W35-W40 N45-N49
2 902 1690 (N50W17 L= 96) 428 126 1 ( 875/1633- 949/1722) 20.0 W11-W22 N46-N51
3 1667 1628 (N19W70 L=150) 1722 174 3 (1625/1554-1705/1687) 48.8 W65-W76 N14-N22
4 1043 1431 (N29W13 L= 93) 357 148 0 ( 981/1390-1098/1469) -58.0 W10-W15 N24-N32
5 487 1358 (N40E28 L= 52) 584 152 1 ( 455/1291- 521/1429) -70.0 E31-E25 N34-N45
6 798 1270 (N26E07 L= 73) 540 173 3 ( 707/1244- 874/1294) -31.0 E12-E02 N23-N29
7 419 1199 (N31E36 L= 44) 263 78 1 ( 390/1167- 436/1228) -76.0 E38-E34 N29-N33
8 1893 1168 (S12W66 L=146) 946 82 0 (1847/1148-1935/1186) -7.1 W59-W75 S14-S10
9 459 1140 (N27E33 L= 47) 451 96 5 ( 408/1109- 500/1173) -14.0 E37-E29 N24-N28
10 553 1078 (N21E27 L= 53) 394 93 1 ( 532/1044- 578/1114) -76.0 E28-E25 N19-N23
11 355 953 (N18E45 L= 35) 828 289 0 ( 274/ 853- 471/1032) -45.0 E51-E37 N10-N24
12 626 943 (N12E25 L= 55) 258 96 0 ( 594/ 902- 664/ 983) -71.6 E26-E23 N08-N14
13 501 874 (N11E35 L= 45) 770 136 4 ( 473/ 798- 541/ 932) 63.4 E38-E32 N06-N14
14 1545 770 (S23W24 L=104) 1011 388 0 (1408/ 669-1654/ 912) 17.7 W13-W35 S25-S17
15 1380 807 (S15W14 L= 94) 236 46 2 (1357/ 785-1410/ 824) 18.4 W13-W16 S16-S13
16 1799 758 (S33W48 L=127) 829 107 1 (1751/ 719-1840/ 792) 5.2 W41-W53 S34-S31
17 1230 620 (S22W01 L= 81) 453 196 0 (1172/ 562-1286/ 706) 31.0 E04-W06 S24-S18
18 725 370 (S24E40 L= 40) 1411 348 1 ( 619/ 251- 809/ 465) 17.8 E58-E30 S31-S18
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Download FITS filament maps as tar archive
» All Filament Data of 20221005 ...
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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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