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| 20130504 - Filament data for 10 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
1 573 1784 (N32E64 L= 76) 1548 132 1 ( 549/1715- 600/1844) -30.1 E78-E57 N26-N37
2 1513 1693 (N56W20 L=160) 1308 116 3 (1463/1642-1547/1739) -71.6 W13-W24 N50-N61
3 1224 1654 (N41E06 L=134) 398 101 0 (1168/1632-1263/1669) 7.1 E10-E02 N39-N42
4 1624 1570 (N49W32 L=172) 444 35 0 (1602/1551-1649/1587) 9.5 W29-W35 N46-N51
5 921 1465 (N19E18 L=122) 1195 253 2 ( 870/1375- 982/1586) -35.5 E25-E11 N14-N25
6 703 1562 (N20E35 L=105) 274 13 0 ( 685/1539- 722/1583) -33.7 E36-E33 N18-N21
7 374 1530 (N10E60 L= 80) 1208 152 3 ( 317/1485- 435/1582) 58.0 E64-E55 N06-N14
8 408 1487 (N08E54 L= 86) 1298 215 4 ( 323/1442- 458/1557) 52.1 E60-E50 N04-N13
9 1355 1517 (N35W08 L=148) 363 72 0 (1319/1488-1388/1540) -9.5 W04-W10 N33-N36
10 1070 1264 (N11E03 L=137) 211 26 0 (1054/1241-1091/1285) -45.0 E04-E02 N09-N12
11 1681 1157 (N21W39 L=179) 469 90 0 (1630/1137-1723/1172) 7.1 W34-W42 N20-N22
12 1676 971 (N10W42 L=182) 370 89 0 (1657/ 941-1702/ 998) -33.7 W40-W44 N08-N12
13 405 831 (S30E37 L=103) 347 83 0 ( 374/ 809- 445/ 861) -18.4 E39-E33 S31-S28
14 733 799 (S24E12 L=128) 375 127 0 ( 684/ 782- 796/ 826) 15.9 E15-E08 S25-S21
15 739 747 (S27E10 L=130) 540 222 0 ( 653/ 717- 852/ 780) 33.7 E15-E03 S30-S22
16 1655 582 (S11W55 L=195) 403 46 0 (1639/ 552-1673/ 608) 90.0 W53-W56 S13-S09
17 1441 567 (S18W39 L=179) 435 53 0 (1417/ 537-1461/ 600) -36.9 W37-W41 S19-S16
18 892 522 (S37W06 L=146) 422 67 1 ( 857/ 504- 932/ 550) 36.9 W03-W08 S38-S35
19 1498 420 (S25W53 L=193) 508 60 0 (1464/ 402-1538/ 440) 7.1 W49-W57 S25-S24
20 972 281 (S52W26 L=166) 499 50 0 ( 947/ 254- 996/ 316) -29.7 W22-W29 S53-S49
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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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