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| 20140320 - Filament data for 08 UTC |
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Available data for 20140320: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1484 1717 (N53W12 L=249) 489 59 0 (1456/1689-1509/1740) -38.7 W08-W14 N50-N55
2 523 1649 (N17E52 L=186) 476 168 0 ( 483/1604- 542/1686) -24.0 E57-E48 N14-N19
3 466 1629 (N15E56 L=182) 406 54 1 ( 439/1609- 498/1647) 45.0 E57-E53 N13-N16
4 397 1528 (N07E56 L=182) 1338 228 2 ( 324/1491- 491/1583) 30.3 E63-E49 N04-N11
5 1003 1515 (N20E15 L=222) 366 103 2 ( 964/1489-1056/1539) 21.8 E17-E11 N18-N21
6 1315 1364 (N20W07 L=245) 424 130 0 (1282/1291-1338/1426) -49.4 W04-W10 N16-N23
7 201 1244 (S13E64 L=174) 2434 265 3 ( 144/1161- 237/1359) 90.0 E68-E59 S18-S05
8 701 1186 (S06E22 L=215) 428 128 2 ( 640/1158- 762/1208) 20.6 E26-E18 S07-S04
9 507 959 (S23E30 L=208) 255 114 1 ( 459/ 933- 560/ 993) 35.5 E33-E26 S25-S20
10 508 832 (S31E28 L=210) 870 234 2 ( 426/ 811- 629/ 872) 10.6 E34-E18 S32-S27
11 845 756 (S27E03 L=234) 409 104 1 ( 784/ 733- 896/ 774) 8.1 E07-W00 S28-S24
12 1183 740 (S18W17 L=255) 1143 390 2 ( 991/ 701-1365/ 768) 19.2 W05-W28 S22-S14
13 1688 628 (S08W55 L=292) 607 108 1 (1665/ 576-1716/ 675) -80.5 W51-W56 S11-S05
14 1588 637 (S11W46 L=284) 452 107 0 (1536/ 613-1628/ 674) 45.0 W42-W48 S13-S08
15 1331 567 (S23W33 L=270) 1891 613 0 (1064/ 476-1540/ 626) 14.4 W15-W50 S30-S16
16 1673 483 (S16W62 L=300) 533 46 0 (1646/ 459-1704/ 511) 53.1 W60-W63 S17-S13
17 1652 398 (S21W66 L=304) 983 249 3 (1618/ 359-1688/ 448) -5.2 W59-W71 S22-S18
18 1203 422 (S35W32 L=270) 558 136 1 (1123/ 406-1268/ 443) 21.8 W26-W36 S37-S32
19 1383 289 (S37W53 L=290) 378 158 0 (1349/ 251-1407/ 328) -12.5 W48-W57 S37-S35
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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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