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| 20140417 - Filament data for 11 UTC |
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Available data for 20140417: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 441 1622 (N14E59 L=168) 1890 370 6 ( 330/1533- 548/1698) 51.8 E64-E51 N06-N21
2 648 1613 (N19E41 L=185) 593 268 0 ( 617/1523- 687/1696) -35.5 E48-E34 N13-N23
3 964 1582 (N25E20 L=206) 314 58 0 ( 941/1552- 986/1615) 90.0 E21-E19 N22-N27
4 604 1427 (N06E36 L=190) 488 101 1 ( 557/1406- 648/1449) 31.0 E39-E33 N04-N08
5 1519 1284 (N23W22 L=248) 825 190 2 (1453/1200-1557/1384) -38.7 W15-W25 N19-N27
6 1216 1294 (N15W03 L=230) 400 139 0 (1162/1236-1247/1356) 77.5 W01-W04 N10-N19
7 487 1194 (S10E37 L=190) 575 177 0 ( 452/1107- 510/1284) -73.3 E38-E35 S14-S04
8 356 1074 (S19E44 L=183) 642 219 0 ( 282/1046- 439/1110) 26.6 E50-E37 S21-S15
9 754 1015 (S13E15 L=211) 316 146 0 ( 692/ 969- 818/1037) 49.4 E17-E11 S17-S10
10 1272 784 (S12W21 L=247) 229 68 1 (1233/ 767-1302/ 799) 26.6 W18-W22 S12-S10
11 268 761 (S41E48 L=178) 636 136 1 ( 230/ 739- 316/ 791) 6.3 E52-E43 S42-S38
12 847 754 (S25E03 L=224) 214 68 0 ( 833/ 715- 860/ 790) -53.1 E03-W00 S27-S22
13 1058 681 (S23W12 L=238) 591 186 2 ( 974/ 652-1133/ 726) 15.3 W06-W17 S26-S18
14 944 591 (S32W09 L=235) 1101 292 2 ( 812/ 514-1090/ 687) 0.0 E02-W20 S34-S29
15 1567 574 (S14W48 L=274) 701 119 1 (1528/ 523-1617/ 604) 66.8 W45-W51 S17-S10
16 1433 308 (S32W55 L=281) 400 48 1 (1410/ 287-1456/ 324) 33.7 W52-W56 S33-S30
17 1062 241 (S51W38 L=264) 2324 347 5 (1008/ 164-1119/ 323) -26.6 W28-W48 S56-S45
18 1360 270 (S37W53 L=279) 696 114 1 (1339/ 232-1388/ 305) -33.7 W49-W55 S39-S35
19 1197 236 (S46W46 L=272) 996 152 2 (1157/ 192-1257/ 275) 12.5 W41-W51 S48-S43
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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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