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| 20240630 - Latest Filament data |
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Available data for 20240630: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1582 1636 (N45W53 L= 46) 730 61 1 (1554/1614-1614/1660) -21.8 W48-W56 N43-N46
2 741 1547 (N35E24 L=329) 343 51 0 ( 722/1516- 762/1580) -45.0 E26-E21 N33-N37
3 1726 1472 (N33W59 L= 52) 726 66 1 (1692/1440-1753/1496) -45.0 W55-W63 N30-N34
4 1056 1463 (N31W01 L=354) 502 226 0 ( 971/1405-1145/1495) -20.0 E05-W06 N27-N32
5 1473 1438 (N30W32 L= 25) 416 191 0 (1398/1391-1547/1465) -9.5 W25-W37 N27-N32
6 1047 1384 (N25W00 L=353) 483 230 0 ( 961/1303-1124/1435) -38.7 E05-W05 N20-N28
7 219 1259 (N13E64 L=290) 1843 135 6 ( 173/1211- 256/1309) 39.8 E71-E59 N10-N16
8 1325 1202 (N15W19 L= 12) 383 145 1 (1258/1171-1375/1241) -26.6 W14-W22 N12-N16
9 1823 921 (S02W59 L= 52) 1064 136 2 (1791/ 870-1863/ 980) -40.6 W55-W64 S05-N01
10 672 871 (S08E22 L=331) 371 159 2 ( 640/ 806- 701/ 929) 82.9 E23-E19 S12-S04
11 1271 798 (S10W16 L= 9) 640 207 1 (1206/ 733-1335/ 884) -48.4 W11-W20 S14-S05
12 1819 779 (S11W62 L= 55) 530 70 1 (1799/ 749-1839/ 815) 68.2 W59-W64 S13-S08
13 280 688 (S22E57 L=296) 498 88 3 ( 266/ 647- 295/ 732) 45.0 E60-E54 S24-S19
14 1081 644 (S21W05 L=358) 857 201 2 (1021/ 557-1133/ 728) -74.7 W01-W09 S26-S15
15 1197 662 (S19W12 L= 6) 652 160 3 (1147/ 591-1226/ 710) -69.4 W09-W14 S24-S16
16 572 530 (S31E32 L=321) 1348 234 3 ( 519/ 474- 665/ 616) -37.9 E35-E24 S35-S25
17 274 572 (S30E64 L=289) 2038 100 3 ( 217/ 540- 316/ 601) 9.8 E85-E56 S33-S27
18 948 539 (S29E04 L=349) 605 143 2 ( 873/ 509- 994/ 575) 32.0 E08-W00 S31-S25
19 1617 483 (S31W51 L= 44) 1672 295 2 (1474/ 431-1721/ 540) 20.0 W38-W61 S35-S27
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Download FITS filament maps as tar archive
» All Filament Data of 20240630 ...
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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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