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| 20140707 - Filament data for 12 UTC |
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Available data for 20140707: »05 UTC »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
1 811 1281 (N19E14 L=220) 492 99 1 ( 782/1249- 855/1321) -45.0 E16-E11 N17-N21
2 1542 1257 (N17W35 L=270) 510 168 1 (1506/1185-1565/1319) 77.5 W33-W36 N12-N21
3 1366 1279 (N19W23 L=257) 311 83 0 (1327/1250-1406/1299) 18.4 W19-W25 N17-N20
4 1428 1158 (N11W26 L=260) 479 167 0 (1366/1133-1511/1198) -12.5 W21-W31 N09-N14
5 1635 1129 (N09W41 L=276) 296 56 0 (1617/1101-1651/1165) 76.0 W39-W42 N07-N11
6 134 1125 (N07E74 L=161) 759 166 1 ( 115/1099- 159/1159) -12.5 E78-E68 N05-N08
7 353 955 (S02E46 L=188) 1313 246 3 ( 283/ 894- 435/1016) -8.7 E52-E39 S05-N01
8 787 975 (N00E15 L=220) 296 62 0 ( 766/ 937- 804/1007) -71.6 E16-E13 S01-N02
9 1434 851 (S07W26 L=261) 224 83 0 (1416/ 816-1468/ 877) 53.1 W25-W28 S09-S05
10 1022 800 (S10E00 L=234) 475 169 2 ( 978/ 726-1071/ 874) 68.2 E02-W02 S15-S05
11 1756 777 (S13W53 L=287) 1121 133 1 (1719/ 713-1791/ 847) 71.6 W49-W56 S17-S08
12 1499 781 (S12W31 L=266) 225 91 0 (1476/ 749-1519/ 834) -71.6 W29-W32 S14-S08
13 652 681 (S18E25 L=210) 307 68 0 ( 613/ 649- 686/ 711) -38.7 E27-E22 S20-S16
14 1408 584 (S25W27 L=261) 257 75 0 (1389/ 551-1423/ 629) 90.0 W25-W27 S27-S21
15 1127 581 (S25W07 L=241) 236 81 0 (1087/ 542-1166/ 607) 38.7 W04-W09 S27-S22
16 1629 583 (S26W45 L=279) 491 105 0 (1588/ 564-1664/ 604) 0.0 W41-W47 S27-S24
17 302 532 (S31E59 L=176) 554 108 1 ( 289/ 501- 329/ 559) 68.2 E61-E55 S33-S28
18 364 471 (S35E55 L=180) 524 85 1 ( 347/ 436- 381/ 503) 78.7 E56-E53 S37-S32
19 1080 405 (S38W04 L=239) 477 78 0 (1037/ 376-1124/ 438) 26.6 W01-W07 S40-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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