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| 20221031 - Latest Filament data |
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Available data for 20221031: »06 UTC »07 UTC »08 UTC »09 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
1 834 1819 (N62W19 L=113) 366 70 0 ( 807/1795- 866/1842) 10.3 W14-W25 N60-N63
2 1159 1806 (N47W43 L=137) 347 41 1 (1140/1783-1184/1826) 0.0 W39-W46 N45-N48
3 1411 1742 (N34W55 L=149) 932 93 3 (1364/1717-1458/1766) -63.4 W50-W58 N31-N37
4 968 1708 (N47W20 L=115) 257 52 0 ( 939/1687- 996/1722) -53.1 W18-W21 N44-N48
5 801 1615 (N46W03 L= 97) 244 63 1 ( 782/1583- 826/1642) -80.5 W01-W04 N42-N48
6 997 1383 (N25W08 L=102) 195 84 0 ( 975/1342-1022/1423) -90.0 W07-W08 N22-N28
7 563 1400 (N38E21 L= 73) 296 81 1 ( 526/1376- 601/1419) -26.6 E24-E18 N35-N39
8 272 1393 (N45E53 L= 41) 688 75 1 ( 231/1376- 312/1415) -13.0 E60-E47 N43-N46
9 513 1243 (N29E27 L= 67) 220 99 0 ( 496/1211- 544/1267) 45.0 E28-E24 N27-N30
10 223 1105 (N27E56 L= 39) 2097 258 7 ( 187/1019- 284/1218) -58.4 E60-E49 N21-N34
11 397 1122 (N25E38 L= 56) 429 106 1 ( 357/1100- 449/1150) 0.0 E41-E33 N23-N26
12 285 881 (N13E52 L= 42) 578 97 3 ( 256/ 837- 307/ 923) 68.2 E54-E49 N10-N15
13 1178 852 (S09W04 L= 99) 408 155 0 (1153/ 774-1213/ 916) 45.0 W01-W07 S12-S06
14 1758 655 (S39W45 L=139) 989 150 1 (1695/ 624-1828/ 679) -3.6 W37-W54 S40-S35
15 934 484 (S24E20 L= 74) 297 119 1 ( 875/ 471- 991/ 502) -14.0 E24-E16 S25-S22
16 824 407 (S27E31 L= 64) 246 100 1 ( 799/ 365- 856/ 440) 39.8 E33-E27 S29-S24
17 477 300 (S26E68 L= 26) 735 75 0 ( 438/ 282- 513/ 320) 5.7 E81-E61 S27-S25
18 1253 254 (S52E10 L= 84) 801 109 1 (1207/ 233-1312/ 276) -24.0 E14-E04 S54-S49
19 1140 175 (S56E27 L= 68) 542 68 0 (1112/ 156-1167/ 200) 20.6 E30-E21 S58-S53
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Download FITS filament maps as tar archive
» All Filament Data of 20221031 ...
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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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