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| 20240712 - Latest Filament data |
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Available data for 20240712: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1219 1652 (N45W20 L=213) 326 80 0 (1181/1636-1262/1671) -23.2 W16-W23 N43-N46
2 1387 1546 (N36W31 L=224) 448 62 3 (1350/1518-1420/1570) -45.0 W28-W33 N34-N38
3 380 1302 (N22E47 L=147) 477 96 0 ( 341/1270- 408/1326) 9.5 E50-E43 N19-N23
4 1025 1262 (N19W01 L=194) 242 130 0 ( 989/1214-1066/1313) -60.3 E01-W03 N15-N22
5 258 1192 (N15E57 L=137) 1258 191 2 ( 233/1104- 283/1271) -84.3 E60-E54 N09-N19
6 1621 1030 (N02W39 L=233) 277 52 1 (1592/1009-1645/1054) 14.0 W37-W41 N00-N03
7 842 877 (S05E12 L=182) 996 290 5 ( 729/ 783- 940/ 977) -45.0 E18-E05 S10-N01
8 1516 867 (S08W31 L=225) 621 125 1 (1479/ 814-1556/ 910) 45.0 W28-W34 S10-S05
9 1353 778 (S12W20 L=214) 561 184 2 (1296/ 717-1379/ 837) 54.5 W16-W22 S16-S08
10 528 699 (S15E34 L=159) 1604 301 4 ( 419/ 631- 645/ 774) -13.2 E42-E25 S19-S10
11 923 588 (S23E08 L=186) 1092 279 0 ( 844/ 485-1021/ 674) 45.0 E14-E01 S30-S17
12 1512 587 (S26W34 L=227) 988 248 3 (1426/ 526-1628/ 643) 21.8 W27-W42 S30-S22
13 665 588 (S23E26 L=168) 598 162 2 ( 616/ 526- 719/ 629) -54.5 E29-E22 S27-S20
14 578 560 (S25E33 L=160) 313 58 1 ( 562/ 531- 596/ 590) -76.0 E34-E32 S26-S22
15 1511 497 (S32W36 L=230) 780 154 0 (1456/ 432-1549/ 555) 60.9 W32-W38 S37-S28
16 800 375 (S39E20 L=173) 471 37 1 ( 772/ 355- 829/ 396) 11.3 E22-E17 S40-S37
17 1241 319 (S46W16 L=210) 987 111 2 (1195/ 284-1295/ 351) -12.5 W12-W21 S49-S42
18 858 223 (S54E22 L=172) 576 63 2 ( 824/ 199- 885/ 249) 7.1 E25-E17 S57-S51
19 1032 197 (S58E03 L=190) 469 42 1 (1011/ 177-1060/ 219) -31.0 E05-W00 S60-S55
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Download FITS filament maps as tar archive
» All Filament Data of 20240712 ...
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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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