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| 20231219 - Filament data for 11 UTC |
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Available data for 20231219: »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
1 655 1529 (N34E22 L= 10) 4818 705 12 ( 392/1320- 900/1678) -30.7 E59-E05 N17-N49
2 1683 1520 (N24W55 L= 87) 414 31 2 (1662/1496-1704/1544) 56.3 W52-W57 N22-N25
3 1206 1455 (N23W16 L= 48) 468 181 1 (1143/1401-1289/1509) -45.0 W12-W20 N19-N27
4 352 1459 (N32E48 L=344) 397 58 0 ( 326/1433- 384/1483) 45.0 E51-E45 N30-N33
5 427 1437 (N29E40 L=352) 319 94 0 ( 388/1407- 456/1460) -15.9 E43-E36 N27-N31
6 400 1307 (N21E41 L=352) 724 191 2 ( 374/1256- 449/1398) -63.4 E43-E36 N17-N27
7 247 1268 (N20E55 L=337) 1093 150 4 ( 219/1201- 280/1333) 66.8 E58-E51 N16-N24
8 186 1207 (N17E62 L=331) 816 136 4 ( 153/1138- 211/1259) -82.9 E66-E59 N12-N20
9 479 1153 (N11E34 L=359) 531 245 3 ( 417/1079- 569/1226) 24.4 E38-E27 N06-N15
10 308 1203 (N15E48 L=344) 329 41 1 ( 285/1177- 334/1224) -45.0 E50-E45 N13-N16
11 337 1115 (N10E45 L=347) 705 139 2 ( 291/1092- 410/1150) -16.7 E49-E39 N07-N12
12 141 1077 (N10E67 L=326) 2322 184 8 ( 93/ 985- 209/1131) -39.3 E77-E57 N04-N13
13 790 762 (S15E17 L= 16) 806 318 2 ( 695/ 653- 879/ 872) 42.7 E24-E10 S21-S09
14 510 724 (S15E36 L=356) 1435 298 1 ( 481/ 582- 545/ 837) 69.4 E39-E31 S24-S08
15 1474 732 (S23W27 L= 60) 1058 288 3 (1380/ 680-1584/ 832) -32.0 W20-W36 S26-S15
16 1656 789 (S20W41 L= 74) 510 84 0 (1615/ 769-1709/ 805) 7.1 W38-W46 S21-S19
17 1682 477 (S42W54 L= 87) 534 57 0 (1652/ 453-1715/ 503) -18.4 W49-W61 S43-S39
18 360 454 (S31E63 L=330) 550 56 0 ( 345/ 415- 376/ 481) 29.1 E67-E58 S33-S28
19 621 435 (S35E37 L=355) 273 29 0 ( 604/ 411- 640/ 456) 36.9 E39-E35 S36-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20231219 ...
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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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