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| 20231129 - Filament data for 11 UTC |
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Available data for 20231129: »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 1213 1899 (N56W53 L=349) 758 66 1 (1193/1861-1228/1931) 19.3 W45-W65 N52-N59
2 1232 1701 (N39W31 L=327) 1346 202 1 (1122/1667-1326/1730) -10.0 W21-W38 N35-N41
3 1553 1614 (N27W52 L=348) 912 190 1 (1477/1559-1628/1655) -45.0 W46-W55 N22-N30
4 1523 1526 (N22W44 L=340) 1095 189 2 (1469/1472-1595/1567) -53.1 W39-W48 N17-N25
5 1453 1457 (N19W36 L=332) 386 47 1 (1432/1428-1475/1493) 76.0 W34-W37 N17-N21
6 935 1467 (N29W02 L=298) 1730 528 1 ( 690/1436-1178/1490) -15.7 E14-W18 N24-N34
7 1382 1399 (N17W29 L=325) 604 190 0 (1292/1379-1465/1418) -14.0 W23-W35 N14-N18
8 598 1377 (N30E22 L=274) 313 94 0 ( 548/1354- 634/1395) -26.6 E25-E19 N27-N30
9 363 1339 (N31E42 L=254) 1138 237 1 ( 262/1296- 456/1389) -15.9 E54-E33 N27-N35
10 1013 1351 (N20W05 L=301) 271 83 0 ( 972/1337-1058/1365) -21.8 W02-W07 N19-N21
11 942 1253 (N16E01 L=295) 957 343 0 ( 811/1176-1088/1330) -45.0 E07-W06 N09-N22
12 1732 1159 (S03W49 L=344) 512 58 0 (1695/1136-1762/1183) 0.0 W45-W51 S04-S01
13 1860 1067 (S11W60 L=356) 573 129 0 (1848/1002-1871/1135) 76.0 W58-W62 S14-S06
14 764 970 (N02E16 L=280) 234 67 1 ( 733/ 954- 796/ 989) 0.0 E18-E13 N01-N03
15 1599 930 (S14W35 L=330) 231 91 0 (1557/ 905-1638/ 959) 9.5 W31-W37 S15-S13
16 1211 757 (S18W07 L=302) 230 59 0 (1189/ 731-1240/ 782) 56.3 W05-W08 S19-S16
17 1254 751 (S19W09 L=305) 211 48 0 (1231/ 728-1283/ 772) 14.0 W07-W11 S20-S17
18 988 718 (S16E07 L=288) 355 124 0 ( 945/ 684-1050/ 760) -54.5 E09-E04 S19-S12
19 1043 493 (S31E09 L=287) 1237 230 1 (1006/ 391-1094/ 616) 57.3 E13-E03 S38-S24
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Download FITS filament maps as tar archive
» All Filament Data of 20231129 ...
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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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