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| 20150611 - Filament data for 14 UTC |
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Available data for 20150611: »06 UTC »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 1075 1614 (N39E06 L= 74) 396 66 1 (1042/1592-1117/1636) -15.9 E08-E01 N37-N41
2 737 1531 (N28E28 L= 52) 767 252 1 ( 674/1449- 822/1612) -31.0 E34-E19 N24-N33
3 427 1429 (N17E48 L= 32) 2561 467 5 ( 370/1260- 481/1573) -42.0 E59-E39 N07-N26
4 1108 1496 (N31E01 L= 79) 334 106 0 (1092/1450-1120/1546) -80.5 E02-W00 N28-N34
5 1690 1467 (N38W47 L=127) 431 76 1 (1657/1443-1713/1488) -21.8 W43-W49 N36-N39
6 930 1369 (N20E11 L= 69) 254 86 0 ( 881/1355- 970/1382) 11.3 E13-E08 N19-N21
7 1193 1277 (N18W07 L= 87) 224 100 1 (1160/1232-1211/1325) -59.0 W04-W08 N15-N20
8 1753 1220 (N22W50 L=129) 1186 296 0 (1675/1105-1835/1322) -36.9 W42-W58 N15-N27
9 1118 1221 (N14W03 L= 83) 206 88 0 (1070/1211-1161/1236) 11.3 W00-W05 N12-N14
10 730 1157 (N05E20 L= 60) 305 115 0 ( 671/1144- 783/1178) 23.2 E23-E16 N03-N06
11 1658 1105 (N13W41 L=121) 468 113 1 (1644/1054-1674/1167) -81.9 W40-W42 N10-N17
12 1743 1103 (N14W49 L=129) 364 93 0 (1719/1065-1761/1136) 59.0 W46-W50 N11-N16
13 209 999 (S12E59 L= 21) 1317 453 4 ( 113/ 968- 312/1025) 4.4 E74-E48 S13-S08
14 790 941 (S07E13 L= 67) 258 109 0 ( 763/ 883- 830/ 987) 74.1 E14-E11 S11-S04
15 1721 653 (S13W56 L=136) 553 100 1 (1681/ 623-1750/ 671) 0.0 W51-W58 S15-S12
16 1320 432 (S33W31 L=111) 289 71 0 (1298/ 414-1346/ 461) -31.0 W28-W33 S34-S31
17 1205 422 (S36W23 L=103) 424 52 2 (1180/ 401-1233/ 448) -11.3 W20-W25 S37-S33
18 1112 421 (S37W16 L= 96) 341 46 0 (1082/ 405-1136/ 442) 45.0 W14-W18 S38-S35
19 477 409 (S49E40 L= 40) 524 140 0 ( 445/ 386- 518/ 433) 24.4 E45-E34 S52-S46
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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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