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| 20260328 - Filament data for 14 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
1 907 1769 (N34E34 L=205) 807 167 0 ( 836/1723- 962/1824) 85.2 E35-E31 N28-N40
2 456 1629 (N14E57 L=182) 1756 207 6 ( 380/1553- 543/1712) -85.2 E64-E52 N08-N20
3 431 1675 (N16E63 L=175) 497 45 1 ( 405/1657- 452/1693) 45.0 E66-E60 N14-N17
4 1065 1665 (N31E18 L=220) 246 65 0 (1031/1647-1096/1682) 53.1 E19-E16 N29-N33
5 518 1555 (N10E47 L=192) 831 160 1 ( 460/1492- 588/1610) 66.0 E49-E44 N05-N14
6 689 1539 (N13E35 L=204) 509 137 1 ( 655/1480- 730/1604) -33.7 E39-E30 N10-N16
7 336 1468 (N01E58 L=180) 357 65 0 ( 313/1450- 362/1494) -9.5 E61-E55 N00-N02
8 216 1058 (S24E57 L=181) 1084 157 5 ( 175/ 994- 250/1116) 53.1 E62-E54 S28-S20
9 303 1004 (S26E47 L=191) 527 123 0 ( 280/ 940- 330/1060) 69.4 E48-E45 S29-S21
10 217 969 (S30E57 L=182) 880 151 1 ( 180/ 891- 248/1023) 66.0 E61-E52 S34-S25
11 854 869 (S20E05 L=233) 323 100 2 ( 830/ 822- 883/ 904) 90.0 E06-E03 S22-S17
12 1820 834 (N08W57 L=296) 566 88 0 (1796/ 789-1843/ 876) -23.2 W53-W61 N06-N09
13 890 769 (S24E00 L=238) 209 57 0 ( 864/ 742- 919/ 794) -14.0 E02-W02 S25-S22
14 388 711 (S42E37 L=202) 438 104 0 ( 342/ 697- 436/ 725) 5.7 E41-E31 S43-S40
15 1226 650 (S21W23 L=261) 685 201 0 (1129/ 621-1331/ 686) 41.6 W17-W27 S24-S15
16 610 655 (S39E16 L=223) 236 39 0 ( 596/ 630- 624/ 683) 71.6 E17-E14 S40-S37
17 1749 658 (S04W58 L=297) 456 77 2 (1718/ 630-1785/ 682) 45.0 W55-W61 S05-S01
18 681 645 (S38E10 L=228) 406 57 0 ( 642/ 625- 712/ 669) 21.8 E12-E07 S39-S35
19 1524 409 (S24W56 L=294) 1202 236 2 (1422/ 382-1634/ 432) 25.2 W48-W66 S28-S19
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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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