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| 20140414 - Filament data for 09 UTC |
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Available data for 20140414: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1440 1712 (N52W07 L=274) 371 66 1 (1415/1684-1459/1735) -9.5 W03-W09 N50-N55
2 899 1679 (N29E29 L=238) 355 70 1 ( 870/1656- 933/1700) -9.5 E31-E25 N27-N30
3 624 1530 (N12E39 L=228) 597 140 2 ( 562/1487- 681/1580) 54.5 E42-E37 N09-N16
4 971 1527 (N21E18 L=249) 570 135 0 ( 936/1467-1007/1580) -29.1 E22-E13 N18-N23
5 524 1408 (N03E41 L=226) 246 68 0 ( 506/1378- 541/1433) -36.9 E42-E38 N01-N04
6 445 1354 (S02E45 L=222) 346 95 2 ( 415/1329- 490/1375) 9.5 E47-E41 S03-N00
7 870 1319 (N06E17 L=250) 343 110 1 ( 820/1270- 898/1347) -18.4 E19-E13 N04-N07
8 276 1264 (S10E56 L=211) 847 232 2 ( 205/1204- 347/1300) 36.0 E62-E49 S15-S07
9 741 1239 (S01E22 L=246) 491 174 0 ( 681/1205- 816/1299) 0.0 E26-E17 S02-N00
10 1181 1239 (N10W03 L=270) 196 42 1 (1152/1221-1203/1256) 45.0 W00-W04 N09-N11
11 342 1088 (S19E45 L=222) 2392 480 9 ( 247/ 939- 396/1248) -54.8 E57-E38 S28-S10
12 232 1167 (S17E57 L=210) 573 124 0 ( 199/1123- 279/1212) 63.4 E60-E53 S19-S13
13 643 870 (S24E18 L=249) 226 78 0 ( 599/ 855- 680/ 886) 9.5 E21-E15 S25-S23
14 995 860 (S15W03 L=270) 201 57 0 ( 960/ 842-1031/ 881) 53.1 W01-W04 S17-S13
15 356 851 (S33E40 L=227) 478 124 1 ( 325/ 813- 406/ 877) 29.7 E42-E35 S35-S30
16 905 764 (S23W01 L=268) 652 247 0 ( 779/ 733-1011/ 802) 36.0 E07-W06 S27-S18
17 1583 526 (S16W52 L=319) 460 102 2 (1547/ 483-1612/ 551) -63.4 W48-W54 S17-S13
18 1368 502 (S24W38 L=305) 252 101 0 (1324/ 480-1405/ 523) 8.1 W34-W41 S24-S23
19 730 444 (S49E00 L=267) 491 84 0 ( 701/ 416- 771/ 488) -26.6 E04-W03 S50-S46
20 842 428 (S46W09 L=276) 369 87 1 ( 818/ 396- 873/ 465) 78.7 W06-W11 S48-S43
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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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