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| 20150422 - Filament data for 08 UTC |
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Available data for 20150422: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1099 1817 (N48E26 L=359) 339 41 0 (1071/1803-1125/1833) 14.0 E27-E23 N46-N49
2 406 1681 (N18E67 L=317) 2521 248 5 ( 354/1635- 459/1733) 49.4 E71-E61 N14-N23
3 1155 1707 (N40E14 L= 10) 296 51 0 (1136/1682-1177/1728) -63.4 E16-E13 N38-N42
4 1179 1666 (N38E11 L= 13) 279 51 1 (1161/1640-1197/1689) -78.7 E12-E09 N35-N40
5 592 1597 (N17E45 L=340) 645 197 0 ( 567/1530- 620/1680) -51.3 E48-E39 N12-N22
6 463 1548 (N11E52 L=332) 1082 306 6 ( 397/1454- 530/1630) 85.9 E55-E48 N03-N17
7 1250 1544 (N32E02 L= 23) 835 187 2 (1212/1453-1293/1617) -45.0 E06-W03 N26-N35
8 1785 1404 (N42W45 L= 70) 574 148 2 (1747/1381-1818/1422) 29.1 W40-W49 N39-N44
9 1652 1267 (N27W33 L= 57) 839 205 2 (1599/1168-1681/1367) -54.0 W27-W35 N21-N32
10 1201 1187 (N09W05 L= 30) 242 68 1 (1181/1164-1235/1212) 71.6 W04-W06 N07-N10
11 744 1058 (S10E17 L= 8) 229 85 0 ( 697/1022- 785/1090) 56.3 E18-E14 S13-S07
12 814 1057 (S09E13 L= 12) 185 28 0 ( 796/1035- 831/1082) -33.7 E14-E11 S09-S07
13 1827 915 (N13W56 L= 81) 2281 383 4 (1787/ 769-1873/1053) -43.0 W49-W68 N06-N20
14 1435 969 (N03W25 L= 49) 389 133 1 (1362/ 945-1483/ 994) 45.0 W20-W27 N00-N06
15 1505 948 (N04W30 L= 54) 220 17 0 (1486/ 927-1524/ 968) 71.6 W28-W30 N02-N05
16 1253 796 (S11W19 L= 44) 471 176 0 (1179/ 732-1344/ 827) 52.1 W16-W23 S16-S07
17 179 801 (S39E58 L=326) 740 189 2 ( 136/ 787- 212/ 823) 18.4 E63-E54 S40-S37
18 998 667 (S26W09 L= 33) 618 154 1 ( 910/ 646-1079/ 690) 29.1 W03-W13 S28-S22
19 1166 518 (S29W25 L= 49) 317 60 0 (1133/ 499-1202/ 541) 11.3 W22-W27 S30-S28
20 944 471 (S39W13 L= 38) 574 144 0 ( 880/ 452-1025/ 494) 21.8 W08-W18 S42-S36
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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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