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| 20231128 - Filament data for 08 UTC |
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Available data for 20231128: »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 1207 1899 (N56W53 L= 4) 701 81 0 (1191/1857-1230/1928) 17.5 W45-W64 N52-N59
2 1105 1856 (N55W35 L=346) 655 86 3 (1072/1816-1129/1889) 37.9 W30-W40 N51-N58
3 1070 1639 (N38W17 L=328) 957 168 1 ( 981/1608-1156/1661) -13.0 W10-W23 N36-N40
4 1379 1595 (N29W37 L=348) 709 189 1 (1321/1542-1477/1632) -45.0 W32-W42 N23-N32
5 1356 1493 (N23W31 L=342) 331 104 2 (1320/1461-1405/1513) -9.5 W28-W34 N21-N24
6 1401 1418 (N18W31 L=342) 291 62 1 (1364/1393-1425/1447) 21.8 W28-W33 N16-N19
7 766 1405 (N29E10 L=301) 1019 378 0 ( 588/1381- 946/1420) -16.3 E22-W02 N24-N31
8 1172 1330 (N17W14 L=325) 619 242 0 (1061/1309-1287/1355) -11.3 W07-W22 N14-N18
9 234 1297 (N31E56 L=254) 997 146 1 ( 184/1250- 293/1354) -21.3 E66-E48 N27-N35
10 736 1287 (N22E13 L=298) 256 111 0 ( 677/1269- 789/1300) -23.2 E16-E09 N20-N23
11 625 1227 (N20E21 L=289) 265 56 0 ( 593/1200- 654/1255) -51.3 E23-E19 N17-N22
12 686 1175 (N16E18 L=293) 222 57 0 ( 659/1155- 720/1199) 14.0 E19-E15 N14-N16
13 820 1127 (N11E10 L=301) 305 93 0 ( 772/1092- 856/1163) -51.3 E12-E08 N08-N13
14 524 884 (N01E33 L=278) 405 124 0 ( 473/ 845- 574/ 928) 18.4 E37-E28 N00-N03
15 1879 823 (S27W63 L= 14) 1566 151 2 (1812/ 770-1926/ 876) 13.2 W54-W71 S28-S23
16 1133 739 (S17W01 L=312) 541 123 1 (1082/ 700-1183/ 796) 33.7 E02-W04 S18-S14
17 1013 719 (S16E06 L=305) 311 117 2 ( 978/ 673-1061/ 760) 33.7 E08-E02 S18-S14
18 735 673 (S14E24 L=287) 232 103 0 ( 702/ 633- 774/ 708) -63.4 E25-E22 S17-S11
19 856 446 (S31E23 L=287) 1022 251 2 ( 826/ 333- 908/ 555) 47.1 E29-E16 S38-S24
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Download FITS filament maps as tar archive
» All Filament Data of 20231128 ...
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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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