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| 20130504 - Filament data for 08 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
1 564 1786 (N32E66 L= 75) 1606 113 1 ( 538/1722- 593/1842) -27.8 E78-E58 N26-N36
2 1503 1699 (N56W18 L=159) 1437 115 3 (1453/1654-1536/1747) -66.0 W12-W23 N50-N62
3 1213 1657 (N40E07 L=134) 548 117 1 (1153/1623-1256/1676) 0.0 E11-E02 N39-N41
4 908 1470 (N19E19 L=122) 1273 284 1 ( 850/1363- 972/1591) -34.5 E27-E11 N13-N25
5 1619 1571 (N49W31 L=172) 439 43 0 (1597/1549-1647/1587) 33.7 W28-W35 N46-N51
6 360 1532 (N10E62 L= 79) 1331 169 3 ( 301/1481- 421/1581) 53.1 E66-E56 N06-N14
7 405 1487 (N08E54 L= 87) 926 146 2 ( 360/1447- 438/1547) 81.9 E57-E51 N05-N12
8 1337 1526 (N35W06 L=147) 359 65 1 (1307/1504-1369/1546) -11.3 W03-W08 N32-N36
9 1056 1275 (N11E04 L=137) 190 18 1 (1040/1254-1076/1294) -45.0 E05-E03 N09-N12
10 1664 1164 (N21W37 L=178) 473 89 0 (1614/1144-1708/1185) 6.3 W32-W41 N20-N22
11 398 831 (S30E38 L=103) 360 72 0 ( 371/ 814- 434/ 856) 0.0 E40-E34 S31-S29
12 716 807 (S24E13 L=128) 344 119 0 ( 672/ 791- 776/ 834) 15.9 E16-E09 S25-S21
13 824 769 (S23E05 L=136) 318 152 0 ( 767/ 743- 876/ 793) 33.7 E08-E01 S26-S21
14 662 748 (S29E15 L=126) 331 58 1 ( 639/ 717- 694/ 778) 90.0 E16-E13 S31-S26
15 1646 583 (S12W54 L=195) 439 39 0 (1629/ 558-1667/ 609) 90.0 W52-W56 S13-S09
16 1427 571 (S19W38 L=179) 435 55 0 (1405/ 542-1451/ 604) -36.9 W36-W40 S20-S16
17 878 529 (S37W05 L=146) 405 60 1 ( 843/ 512- 917/ 554) 36.9 W02-W07 S38-S35
18 1485 426 (S25W51 L=192) 523 91 0 (1442/ 409-1530/ 445) 6.3 W46-W55 S26-S23
19 961 285 (S52W25 L=166) 516 39 1 ( 935/ 259- 986/ 319) -29.7 W21-W28 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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