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| 20140112 - Filament data for 12 UTC |
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Available data for 20140112: »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
1 526 1533 (N26E37 L= 0) 1813 370 3 ( 419/1461- 643/1602) -20.9 E48-E27 N21-N31
2 1085 1467 (N23W02 L= 40) 427 85 1 (1033/1434-1131/1488) -9.5 E01-W05 N21-N24
3 1314 1429 (N22W17 L= 55) 281 54 1 (1287/1409-1352/1449) -14.0 W15-W19 N20-N23
4 311 1400 (N17E52 L=345) 335 55 1 ( 287/1385- 333/1420) -26.6 E54-E50 N16-N18
5 1064 1229 (N08W02 L= 39) 257 95 0 (1039/1190-1107/1271) -45.0 W00-W04 N05-N10
6 1817 1152 (N08W55 L= 93) 394 65 1 (1796/1123-1838/1191) -45.0 W52-W57 N06-N10
7 1860 875 (S08W62 L=100) 9243 1379 28 (1783/ 628-1952/1172) -81.1 W52-W75 S22-N10
8 795 1129 (N01E14 L= 24) 258 85 0 ( 757/1099- 839/1148) -75.5 E16-E11 N00-N02
9 699 966 (S09E20 L= 18) 204 79 0 ( 655/ 941- 738/ 990) 31.0 E22-E17 S10-S07
10 288 936 (S11E50 L=348) 415 61 0 ( 268/ 898- 303/ 980) 78.7 E52-E48 S13-S08
11 1446 869 (S11W27 L= 65) 273 71 0 (1428/ 830-1461/ 910) -68.2 W25-W28 S13-S08
12 201 855 (S16E60 L=338) 586 140 0 ( 170/ 816- 245/ 888) 24.0 E63-E54 S17-S13
13 1651 669 (S22W46 L= 83) 1691 373 5 (1592/ 554-1690/ 813) -60.6 W38-W50 S29-S13
14 853 637 (S29E10 L= 28) 1662 282 3 ( 703/ 553-1022/ 750) 31.8 E21-W01 S34-S20
15 537 651 (S28E33 L= 5) 871 221 1 ( 466/ 586- 615/ 739) 36.9 E39-E25 S32-S22
16 279 594 (S32E57 L=341) 1802 337 6 ( 206/ 539- 342/ 633) 0.0 E64-E50 S35-S29
17 616 485 (S40E29 L= 8) 681 142 1 ( 552/ 451- 664/ 525) 20.0 E36-E25 S42-S36
18 1633 444 (S36W52 L= 90) 921 76 0 (1594/ 412-1666/ 485) 59.0 W49-W54 S38-S33
19 1170 450 (S40W14 L= 52) 390 64 1 (1133/ 427-1208/ 473) 21.8 W11-W16 S41-S38
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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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