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| 20230422 - Filament data for 12 UTC |
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Available data for 20230422: »06 UTC »07 UTC »08 UTC »09 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 1367 1705 (N49W01 L=336) 798 113 1 (1338/1659-1402/1744) -40.6 E02-W05 N45-N52
2 584 1572 (N15E44 L=291) 1199 247 4 ( 515/1490- 643/1680) -74.1 E50-E42 N08-N22
3 926 1617 (N27E25 L=311) 333 125 1 ( 886/1570- 953/1671) -29.1 E29-E20 N24-N29
4 1114 1468 (N23E08 L=328) 932 396 5 (1072/1293-1160/1655) -70.2 E12-E03 N11-N36
5 1612 1500 (N42W27 L= 3) 2209 356 3 (1471/1381-1734/1582) -8.4 W13-W40 N38-N45
6 1416 1421 (N29W12 L=348) 292 135 0 (1393/1378-1459/1477) -35.5 W09-W16 N27-N32
7 1386 1304 (N21W13 L=349) 346 170 0 (1305/1257-1447/1333) 5.2 W07-W18 N19-N21
8 212 1141 (S18E61 L=274) 1285 214 5 ( 174/1055- 249/1232) 74.7 E64-E57 S23-S12
9 1452 1162 (N15W21 L=356) 285 152 0 (1435/1088-1466/1230) -58.0 W18-W23 N10-N18
10 1582 1151 (N18W30 L= 5) 561 97 1 (1563/1098-1598/1200) -71.6 W27-W31 N14-N20
11 1266 1108 (N06W11 L=346) 190 81 1 (1238/1075-1285/1145) 78.7 W10-W12 N03-N08
12 1786 883 (N10W54 L= 29) 652 102 2 (1758/ 843-1819/ 929) -23.2 W50-W58 N07-N12
13 973 721 (S23W06 L=341) 1429 474 3 ( 919/ 605-1108/ 901) -39.1 W00-W17 S28-S12
14 590 707 (S35E19 L=316) 788 260 1 ( 471/ 685- 722/ 730) 25.3 E28-E09 S39-S30
15 1172 640 (S22W20 L=356) 234 118 0 (1132/ 621-1237/ 654) 45.0 W18-W23 S24-S19
16 697 548 (S42E07 L=328) 698 157 1 ( 637/ 522- 772/ 589) 41.6 E11-E02 S45-S37
17 505 558 (S48E24 L=311) 321 46 1 ( 479/ 536- 526/ 582) 0.0 E27-E22 S49-S46
18 1508 453 (S22W52 L= 27) 539 105 2 (1469/ 419-1551/ 500) 80.5 W48-W54 S23-S17
19 1633 450 (S18W63 L= 38) 522 100 0 (1587/ 430-1674/ 471) 33.7 W59-W66 S19-S15
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Download FITS filament maps as tar archive
» All Filament Data of 20230422 ...
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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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