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| 20130504 - Filament data for 06 UTC |
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Available data for 20130504: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 556 1787 (N31E67 L= 75) 1677 115 1 ( 530/1724- 585/1840) -29.1 E79-E59 N26-N36
2 1494 1705 (N56W17 L=159) 1569 132 3 (1440/1661-1539/1754) 40.2 W11-W24 N49-N61
3 1198 1660 (N40E08 L=134) 567 128 1 (1138/1628-1248/1680) 0.0 E12-E03 N37-N41
4 365 1547 (N11E62 L= 80) 1580 216 2 ( 302/1487- 418/1617) 73.3 E67-E58 N06-N16
5 891 1483 (N19E20 L=122) 1225 262 1 ( 835/1391- 955/1600) -33.7 E28-E13 N14-N25
6 1606 1573 (N48W30 L=172) 391 36 0 (1576/1557-1627/1590) 33.7 W26-W32 N46-N50
7 401 1494 (N09E55 L= 87) 1098 157 2 ( 355/1451- 445/1563) 76.0 E58-E52 N05-N13
8 1324 1531 (N35W05 L=147) 375 58 1 (1297/1509-1358/1554) -11.3 W02-W07 N32-N35
9 1653 1169 (N21W36 L=178) 456 118 0 (1599/1149-1703/1190) 6.3 W31-W40 N20-N22
10 1646 984 (N10W39 L=181) 263 48 0 (1631/ 956-1662/1010) 90.0 W38-W40 N08-N12
11 391 835 (S30E38 L=104) 260 62 0 ( 363/ 819- 420/ 856) -9.5 E41-E35 S31-S29
12 706 812 (S24E14 L=128) 315 113 0 ( 663/ 797- 764/ 834) 26.6 E16-E10 S25-S21
13 733 764 (S26E11 L=131) 646 328 2 ( 630/ 723- 864/ 800) 29.7 E17-E02 S31-S21
14 1415 575 (S19W37 L=179) 426 61 1 (1394/ 549-1439/ 606) -26.6 W35-W39 S20-S16
15 1627 581 (S12W53 L=195) 399 36 1 (1598/ 560-1652/ 603) 33.7 W50-W55 S13-S10
16 864 535 (S37W04 L=146) 334 59 0 ( 833/ 517- 898/ 558) 45.0 W02-W05 S38-S34
17 1477 429 (S25W51 L=192) 516 81 0 (1433/ 409-1517/ 449) 6.3 W45-W54 S26-S23
18 950 293 (S52W23 L=165) 515 85 1 ( 914/ 266- 974/ 328) 68.2 W20-W26 S53-S48
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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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