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| 20260328 - Filament data for 12 UTC |
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Available data for 20260328: »08 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 892 1752 (N32E34 L=206) 867 153 0 ( 847/1696- 943/1812) -79.7 E35-E31 N27-N38
2 573 1765 (N25E58 L=181) 528 83 0 ( 539/1728- 591/1791) -21.8 E64-E54 N22-N26
3 436 1678 (N16E63 L=176) 781 81 0 ( 395/1658- 473/1697) 26.6 E67-E59 N14-N18
4 425 1609 (N12E58 L=181) 2008 180 6 ( 375/1535- 480/1669) -84.3 E66-E52 N06-N16
5 508 1560 (N10E48 L=191) 776 157 0 ( 452/1502- 571/1612) 69.4 E50-E45 N05-N14
6 698 1506 (N11E33 L=207) 241 35 0 ( 683/1484- 716/1536) -33.7 E34-E31 N10-N12
7 218 1097 (S22E58 L=182) 416 64 1 ( 188/1064- 242/1117) -21.8 E61-E55 S23-S20
8 291 1007 (S26E49 L=191) 743 169 1 ( 265/ 930- 322/1062) 63.4 E50-E46 S30-S22
9 200 1037 (S26E59 L=180) 523 41 0 ( 179/1005- 223/1061) 36.9 E61-E56 S27-S24
10 208 979 (S29E58 L=182) 777 110 1 ( 166/ 938- 240/1025) 33.7 E63-E53 S31-S25
11 839 873 (S20E06 L=233) 369 84 0 ( 814/ 824- 871/ 904) 90.0 E07-E04 S22-S17
12 1813 845 (N08W56 L=295) 558 82 0 (1787/ 800-1836/ 885) -26.6 W52-W60 N06-N10
13 876 779 (S24E01 L=238) 233 87 0 ( 841/ 748- 908/ 810) -11.3 E04-W01 S25-S22
14 384 716 (S42E37 L=203) 524 70 1 ( 336/ 699- 424/ 744) 5.7 E42-E32 S43-S39
15 1217 657 (S21W22 L=262) 726 207 1 (1120/ 628-1318/ 691) 38.7 W17-W27 S24-S16
16 1745 669 (S03W57 L=297) 326 33 1 (1727/ 647-1765/ 687) 56.3 W54-W59 S04-S01
17 596 658 (S39E17 L=223) 271 29 0 ( 575/ 634- 612/ 685) 90.0 E18-E15 S40-S37
18 671 650 (S38E11 L=229) 430 68 1 ( 629/ 626- 707/ 673) 18.4 E14-E08 S39-S35
19 1521 416 (S23W55 L=294) 1236 264 0 (1410/ 396-1642/ 441) 27.9 W47-W65 S27-S18
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Data will be available after one hour of observations. |
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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