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| 20251201 - Latest Filament data |
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Available data for 20251201: »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1119 1588 (N33W17 L=359) 3241 707 6 ( 801/1529-1443/1650) -21.3 E04-W38 N24-N42
2 1568 1612 (N27W51 L= 33) 356 63 2 (1526/1592-1593/1629) -31.0 W48-W54 N25-N28
3 1688 1502 (N18W56 L= 38) 831 137 1 (1624/1468-1735/1542) -32.0 W51-W60 N15-N21
4 1598 1451 (N16W46 L= 27) 265 129 0 (1532/1422-1642/1469) -29.7 W41-W48 N14-N18
5 160 1199 (N24E64 L=278) 6834 362 17 ( 81/1054- 232/1457) -76.5 E79-E53 N15-N41
6 1470 1211 (N05W30 L= 11) 713 130 3 (1440/1138-1495/1274) 82.9 W27-W31 N00-N08
7 1907 1188 (S04W68 L= 50) 568 61 0 (1877/1166-1934/1224) -33.7 W64-W72 S05-S01
8 1731 1052 (S09W46 L= 28) 437 96 2 (1702/1025-1776/1083) -8.1 W43-W50 S10-S06
9 188 933 (N08E60 L=282) 993 170 4 ( 170/ 855- 208/1006) 71.6 E63-E56 N03-N12
10 1723 913 (S17W44 L= 26) 278 48 1 (1702/ 883-1740/ 937) -56.3 W42-W45 S18-S15
11 242 852 (N02E56 L=286) 640 86 2 ( 213/ 812- 271/ 903) 29.7 E59-E51 N00-N05
12 1088 642 (S23E02 L=339) 728 234 2 ( 987/ 583-1165/ 716) 22.6 E09-W03 S24-S19
13 280 585 (S14E62 L=280) 3736 256 7 ( 214/ 484- 338/ 676) 47.7 E70-E53 S19-S08
14 430 497 (S21E52 L=290) 1024 143 3 ( 381/ 430- 463/ 544) 69.4 E56-E47 S25-S17
15 853 447 (S31E22 L=320) 446 85 3 ( 827/ 406- 882/ 489) 51.3 E25-E19 S33-S28
16 1387 403 (S45W16 L=358) 1309 200 4 (1281/ 379-1478/ 439) -6.3 W06-W24 S48-S41
17 1569 412 (S48W35 L= 17) 462 72 0 (1540/ 396-1610/ 438) -24.4 W30-W41 S50-S45
18 692 306 (S38E42 L=300) 405 90 0 ( 649/ 279- 722/ 331) -63.4 E44-E39 S40-S35
19 1242 209 (S60W00 L=342) 2111 282 4 (1108/ 172-1376/ 241) -8.9 E15-W17 S64-S56
20 1015 145 (S60E29 L=313) 726 82 2 ( 980/ 127-1063/ 172) -51.3 E33-E24 S63-S56
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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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