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| 20140108 - Filament data for 11 UTC |
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Available data for 20140108: »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 1351 1519 (N28W21 L=113) 317 56 0 (1314/1496-1381/1540) -31.0 W18-W23 N26-N29
2 335 1445 (N22E51 L= 40) 442 78 1 ( 318/1413- 359/1473) -53.1 E53-E48 N20-N24
3 1391 1447 (N23W23 L=115) 305 52 2 (1357/1427-1418/1469) 26.6 W21-W25 N22-N24
4 523 1439 (N21E35 L= 56) 366 94 1 ( 474/1419- 566/1452) 0.0 E38-E31 N20-N22
5 284 1197 (N06E51 L= 40) 600 146 2 ( 265/1138- 314/1275) -71.6 E53-E48 N02-N11
6 148 1160 (N05E67 L= 24) 1414 184 3 ( 112/1099- 183/1226) 41.2 E73-E62 N01-N08
7 961 1125 (N02E04 L= 87) 534 145 2 ( 926/1080- 985/1196) 71.6 E05-E02 N00-N06
8 1215 1016 (S04W12 L=103) 315 91 1 (1158/ 996-1259/1036) -9.5 W08-W14 S05-S02
9 1039 881 (S12W01 L= 92) 301 91 2 ( 988/ 848-1079/ 917) 45.0 E01-W03 S14-S10
10 1297 877 (S12W17 L=108) 188 84 0 (1253/ 867-1345/ 893) 9.5 W14-W20 S12-S10
11 1774 856 (S11W53 L=144) 444 120 1 (1744/ 812-1796/ 889) -38.7 W49-W55 S13-S09
12 921 735 (S22E06 L= 85) 724 194 0 ( 895/ 634- 949/ 822) 90.0 E07-E04 S28-S16
13 331 786 (S18E48 L= 43) 573 142 3 ( 292/ 748- 369/ 814) 20.6 E52-E44 S20-S16
14 1355 760 (S19W22 L=113) 546 148 1 (1276/ 734-1407/ 800) 18.4 W16-W25 S20-S16
15 625 744 (S21E26 L= 65) 393 99 0 ( 591/ 708- 682/ 775) 23.2 E28-E21 S23-S19
16 1285 655 (S26W18 L=109) 1135 445 3 (1172/ 611-1499/ 743) 9.9 W10-W33 S28-S20
17 257 610 (S29E59 L= 32) 1552 400 2 ( 227/ 510- 290/ 684) 37.6 E66-E53 S35-S24
18 560 542 (S34E34 L= 57) 323 115 1 ( 544/ 493- 579/ 586) 63.4 E36-E31 S37-S31
19 1050 528 (S35W03 L= 94) 325 93 0 (1004/ 492-1088/ 570) 45.0 W00-W05 S37-S31
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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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