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| 20260312 - Filament data for 10 UTC |
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Available data for 20260312: »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 1338 1583 (N34W04 L= 95) 402 65 0 (1309/1551-1370/1612) 71.6 W02-W05 N31-N37
2 643 1544 (N13E37 L= 55) 707 147 2 ( 585/1494- 710/1572) 50.2 E39-E33 N08-N15
3 1627 1414 (N33W28 L=120) 1188 293 2 (1501/1342-1743/1493) -2.6 W17-W39 N30-N34
4 326 1268 (S09E51 L= 41) 454 66 1 ( 293/1241- 356/1301) 53.1 E53-E47 S10-S06
5 545 1103 (S14E30 L= 61) 3304 795 4 ( 237/1031- 866/1230) 11.1 E57-E11 S19-S05
6 142 1176 (S17E70 L= 22) 1084 75 3 ( 110/1135- 168/1209) -24.0 E76-E65 S18-S14
7 1751 1057 (N15W44 L=136) 372 57 0 (1731/1031-1777/1088) -71.6 W42-W46 N13-N17
8 206 987 (S27E58 L= 34) 744 115 0 ( 176/ 932- 233/1036) 50.2 E62-E54 S30-S24
9 1613 887 (N02W38 L=130) 749 109 1 (1580/ 836-1641/ 938) -78.7 W34-W40 S01-N05
10 1824 826 (N06W58 L=149) 787 124 2 (1800/ 760-1847/ 879) -74.1 W55-W60 N01-N08
11 1421 686 (S14W33 L=124) 514 126 0 (1379/ 638-1473/ 741) -18.4 W28-W37 S15-S12
12 463 638 (S44E30 L= 62) 423 57 1 ( 432/ 612- 489/ 669) 38.7 E33-E27 S45-S41
13 1067 586 (S30W16 L=107) 672 151 2 ( 992/ 564-1143/ 621) 21.8 W10-W20 S32-S28
14 599 588 (S44E17 L= 75) 246 59 0 ( 571/ 572- 621/ 608) 14.0 E19-E14 S44-S41
15 811 553 (S40W00 L= 92) 576 134 4 ( 761/ 534- 895/ 580) 24.0 E03-W06 S41-S37
16 1517 486 (S22W49 L=140) 411 74 0 (1498/ 447-1534/ 523) -45.0 W46-W51 S23-S19
17 404 445 (S61E42 L= 49) 734 103 2 ( 367/ 411- 448/ 482) -16.7 E48-E35 S62-S58
18 1330 258 (S40W55 L=147) 491 36 0 (1313/ 228-1347/ 289) -18.4 W50-W59 S42-S38
19 1234 247 (S45W49 L=141) 407 48 2 (1216/ 222-1254/ 275) -14.0 W45-W53 S46-S43
20 1140 219 (S50W46 L=138) 811 120 0 (1102/ 194-1204/ 253) 18.4 W40-W51 S52-S47
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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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