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| 20140127 - Latest Filament data |
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Available data for 20140127: »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 311 1512 (N18E59 L=142) 486 173 0 ( 290/1459- 328/1557) -41.2 E62-E54 N14-N21
2 1156 1489 (N24W03 L=204) 212 67 0 (1120/1474-1193/1507) 11.3 W00-W05 N23-N25
3 204 1332 (N07E64 L=137) 465 163 1 ( 163/1315- 242/1345) -5.2 E70-E59 N05-N07
4 238 1142 (S05E56 L=145) 375 41 0 ( 217/1116- 261/1168) 45.0 E57-E53 S06-S03
5 1184 1056 (S02W09 L=210) 332 116 0 (1120/1025-1244/1076) -8.1 W05-W12 S03-S01
6 1310 944 (S07W18 L=219) 238 51 1 (1283/ 920-1341/ 975) 33.7 W16-W19 S08-S05
7 876 870 (S16E07 L=194) 367 135 1 ( 846/ 799- 908/ 922) 66.8 E08-E05 S20-S13
8 1441 862 (S10W28 L=228) 340 73 1 (1408/ 823-1476/ 905) 68.2 W25-W29 S12-S07
9 1282 840 (S13W18 L=219) 382 165 1 (1181/ 826-1349/ 862) 10.3 W11-W22 S14-S11
10 261 733 (S30E53 L=147) 1668 328 1 ( 212/ 638- 310/ 861) 49.4 E60-E47 S35-S21
11 646 776 (S24E22 L=179) 201 89 0 ( 627/ 727- 660/ 821) 80.5 E22-E20 S27-S21
12 1346 789 (S15W23 L=224) 231 53 1 (1313/ 773-1375/ 810) 14.0 W20-W24 S16-S14
13 1719 700 (S15W52 L=253) 2063 320 1 (1591/ 605-1840/ 792) 37.9 W43-W62 S22-S07
14 1015 697 (S25W03 L=204) 598 183 0 ( 935/ 628-1106/ 732) 37.9 E01-W09 S30-S22
15 1450 671 (S21W32 L=233) 549 177 3 (1383/ 620-1501/ 714) -11.3 W27-W37 S23-S18
16 1210 633 (S27W17 L=218) 386 111 0 (1152/ 606-1269/ 665) 40.6 W13-W20 S29-S23
17 1370 558 (S29W30 L=231) 827 188 0 (1302/ 520-1448/ 628) -9.5 W23-W35 S31-S25
18 1732 457 (S28W64 L=265) 914 108 1 (1692/ 434-1765/ 486) 26.6 W60-W67 S30-S26
19 641 357 (S54E26 L=175) 295 46 0 ( 622/ 331- 660/ 380) -63.4 E28-E24 S56-S52
20 1326 296 (S48W39 L=240) 602 135 0 (1270/ 278-1391/ 315) 18.4 W34-W44 S49-S45
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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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