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| 20251130 - Filament data for 09 UTC |
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Available data for 20251130: »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 1077 1946 (N66W47 L= 43) 673 62 1 (1058/1912-1097/1980) 13.6 W38-W71 N61-N69
2 969 1895 (N63W23 L= 19) 573 54 1 ( 940/1869- 988/1925) 24.8 W17-W30 N60-N66
3 1425 1768 (N40W52 L= 47) 670 98 1 (1380/1746-1474/1783) -5.2 W46-W57 N37-N41
4 933 1537 (N33W03 L=359) 2609 629 5 ( 644/1479-1235/1600) -24.1 E17-W21 N24-N41
5 310 1542 (N46E55 L=300) 727 79 1 ( 268/1516- 348/1561) -7.1 E65-E49 N43-N48
6 1426 1410 (N17W32 L= 27) 282 127 1 (1358/1386-1472/1440) -29.7 W27-W34 N14-N18
7 1243 1143 (N04W14 L= 10) 686 152 2 (1208/1066-1266/1214) 69.4 W12-W16 N00-N08
8 1802 1164 (S04W54 L= 50) 381 69 1 (1760/1151-1841/1179) -14.0 W50-W58 S04-S02
9 1942 986 (S16W71 L= 66) 1198 169 1 (1911/ 899-1963/1061) -47.7 W65-W76 S22-S11
10 1570 981 (S10W33 L= 28) 241 53 0 (1553/ 945-1586/1011) 63.4 W31-W33 S12-S08
11 1895 852 (S24W64 L= 59) 1674 159 2 (1846/ 816-1957/ 892) 3.2 W56-W76 S25-S20
12 1090 760 (S15E00 L=355) 244 56 2 (1068/ 728-1111/ 784) 33.7 E02-W01 S16-S13
13 328 629 (S11E55 L=301) 1278 288 4 ( 267/ 516- 398/ 744) -82.4 E57-E52 S18-S03
14 793 509 (S26E24 L=331) 1917 457 5 ( 655/ 358- 970/ 651) 22.8 E40-E09 S33-S19
15 273 517 (S17E68 L=287) 3154 218 9 ( 195/ 448- 355/ 584) -36.9 E85-E58 S22-S13
16 309 556 (S15E61 L=295) 624 51 2 ( 283/ 536- 335/ 583) -45.0 E64-E57 S16-S13
17 1279 367 (S45W06 L= 2) 1643 266 6 (1141/ 325-1384/ 418) -22.8 E04-W15 S51-S41
18 1153 178 (S61E12 L=343) 2459 306 6 ( 997/ 125-1284/ 215) -2.9 E35-W04 S65-S56
19 932 126 (S60E42 L=313) 484 60 1 ( 912/ 105- 965/ 152) -90.0 E47-E37 S62-S56
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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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