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| 20130504 - Filament data for 09 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
1 568 1784 (N31E65 L= 75) 1673 134 1 ( 543/1715- 597/1846) -29.7 E79-E57 N25-N37
2 1508 1695 (N56W19 L=159) 1428 118 4 (1457/1658-1551/1744) 47.7 W13-W24 N49-N61
3 1219 1654 (N40E06 L=134) 488 121 1 (1158/1620-1263/1671) 0.0 E10-E01 N38-N41
4 696 1563 (N19E36 L=105) 283 19 0 ( 679/1539- 714/1586) -33.7 E37-E34 N17-N21
5 1622 1570 (N49W32 L=172) 410 33 0 (1600/1550-1648/1586) 18.4 W29-W35 N46-N51
6 918 1461 (N19E18 L=123) 1318 252 2 ( 864/1364- 975/1583) -38.2 E25-E11 N13-N25
7 394 1516 (N10E57 L= 83) 2331 286 6 ( 315/1456- 451/1581) 41.2 E65-E50 N05-N14
8 1346 1522 (N35W07 L=147) 343 54 0 (1313/1498-1377/1539) 0.0 W04-W09 N33-N36
9 1063 1269 (N11E04 L=137) 206 23 0 (1048/1246-1084/1288) -45.0 E05-E02 N09-N12
10 1674 1160 (N21W38 L=178) 465 90 0 (1623/1140-1717/1176) 6.3 W33-W42 N20-N22
11 400 834 (S30E37 L=103) 362 95 0 ( 371/ 811- 442/ 870) -8.1 E40-E33 S31-S28
12 727 803 (S24E12 L=128) 381 129 0 ( 676/ 786- 787/ 833) 14.0 E16-E08 S25-S21
13 802 758 (S25E06 L=134) 265 117 0 ( 745/ 737- 849/ 785) 45.0 E09-E04 S26-S21
14 667 745 (S29E15 L=125) 309 48 1 ( 647/ 715- 695/ 775) 90.0 E16-E13 S31-S26
15 1652 584 (S11W55 L=195) 414 44 0 (1634/ 555-1671/ 609) -76.0 W52-W56 S13-S09
16 1434 567 (S19W39 L=179) 437 68 0 (1411/ 533-1455/ 600) -36.9 W36-W41 S19-S16
17 889 526 (S37W06 L=146) 406 44 0 ( 860/ 508- 926/ 550) 21.8 W03-W08 S38-S35
18 1494 421 (S25W52 L=193) 518 75 0 (1457/ 404-1539/ 439) 6.3 W48-W57 S26-S24
19 968 281 (S52W26 L=166) 552 63 0 ( 941/ 253- 998/ 315) -18.4 W21-W30 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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