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| 20241006 - Filament data for 07 UTC |
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Available data for 20241006: »06 UTC »07 UTC »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 1596 1515 (N15W52 L=192) 321 74 1 (1559/1495-1630/1530) -31.0 W50-W55 N14-N17
2 1733 1431 (N07W59 L=199) 583 106 2 (1686/1404-1760/1470) 0.0 W53-W64 N05-N08
3 1078 1402 (N25W14 L=154) 216 58 1 (1041/1383-1106/1423) -53.1 W12-W15 N23-N27
4 1869 1190 (S11W62 L=202) 3438 339 9 (1806/1054-1922/1292) 61.7 W55-W73 S19-S05
5 1013 1252 (N19W06 L=145) 428 127 0 ( 943/1236-1075/1268) -26.6 W01-W09 N16-N21
6 848 1158 (N18E06 L=133) 312 176 1 ( 779/1106- 914/1201) -53.1 E09-E03 N13-N21
7 1692 1156 (S06W44 L=183) 321 72 3 (1673/1127-1718/1185) -76.0 W42-W45 S08-S04
8 1826 1043 (S17W53 L=192) 2345 316 7 (1779/ 868-1866/1155) -87.0 W49-W57 S28-S09
9 278 975 (N21E51 L= 89) 2056 391 2 ( 180/ 833- 362/1151) -54.5 E62-E45 N12-N33
10 1674 1044 (S11W39 L=179) 365 140 0 (1634/1007-1724/1085) 0.0 W35-W43 S12-S09
11 500 974 (N17E33 L=107) 293 114 0 ( 445/ 944- 550/1011) -45.0 E35-E29 N13-N19
12 1227 804 (S11W05 L=145) 648 342 1 (1179/ 646-1247/ 947) 56.3 E01-W09 S18-S03
13 1581 889 (S17W29 L=168) 294 97 0 (1532/ 876-1626/ 900) -33.7 W25-W31 S19-S14
14 1369 562 (S30W07 L=147) 2991 581 8 (1217/ 367-1530/ 782) 31.8 E08-W22 S38-S20
15 1110 677 (S15E05 L=135) 193 107 0 (1063/ 659-1159/ 691) -38.7 E07-E02 S17-S13
16 386 616 (S01E52 L= 88) 1275 194 4 ( 305/ 571- 463/ 680) -18.4 E60-E46 S05-N02
17 559 611 (S05E39 L=101) 880 217 5 ( 505/ 499- 594/ 675) 65.6 E44-E34 S11-N00
18 757 451 (S19E33 L=107) 1021 328 2 ( 735/ 309- 793/ 594) 46.7 E41-E25 S29-S11
19 948 501 (S21E20 L=120) 296 117 1 ( 930/ 449- 960/ 570) 54.5 E22-E16 S24-S17
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Download FITS filament maps as tar archive
» All Filament Data of 20241006 ...
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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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