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| 20230907 - Filament data for 06 UTC |
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Available data for 20230907: »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 1593 1664 (N27W67 L= 20) 1744 137 4 (1529/1604-1647/1707) -76.0 W62-W72 N23-N31
2 1481 1507 (N23W44 L=358) 484 131 1 (1463/1436-1502/1559) 36.9 W40-W48 N18-N25
3 1332 1523 (N28W35 L=348) 246 84 0 (1300/1499-1365/1543) -53.1 W32-W35 N25-N29
4 1612 1497 (N18W54 L= 8) 973 182 1 (1533/1449-1681/1532) -45.0 W49-W58 N13-N22
5 816 1441 (N37E03 L=311) 260 30 1 ( 795/1413- 838/1465) 56.3 E04-E01 N35-N38
6 1287 1346 (N19W24 L=338) 374 105 3 (1238/1321-1337/1380) -26.6 W21-W27 N16-N21
7 985 1226 (N20W02 L=316) 326 135 2 ( 965/1160-1005/1287) 54.5 W00-W05 N15-N22
8 1733 1154 (S04W49 L= 3) 388 91 1 (1713/1110-1762/1198) 45.0 W46-W52 S05-S01
9 184 1077 (N26E65 L=249) 557 58 1 ( 166/1048- 211/1105) 56.3 E67-E60 N24-N27
10 280 1032 (N22E53 L=261) 2236 485 5 ( 155/ 940- 477/1102) 0.0 E69-E34 N17-N26
11 1538 987 (S08W30 L=344) 288 48 1 (1514/ 959-1558/1011) 56.3 W28-W31 S09-S06
12 1825 842 (S26W53 L= 7) 1560 182 2 (1764/ 783-1901/ 895) 6.3 W46-W65 S28-S23
13 1685 852 (S20W39 L=352) 646 196 0 (1587/ 821-1743/ 886) -15.9 W30-W44 S21-S16
14 481 820 (N06E39 L=275) 286 118 1 ( 439/ 778- 511/ 872) -66.8 E40-E37 N03-N10
15 1033 797 (S06E05 L=309) 393 159 1 ( 998/ 722-1067/ 842) 39.8 E08-E02 S09-S02
16 474 700 (S01E42 L=271) 369 118 0 ( 458/ 641- 489/ 757) 50.2 E44-E39 S04-N02
17 1112 534 (S24E07 L=307) 722 241 2 (1043/ 443-1172/ 629) 36.9 E13-W00 S29-S18
18 1371 447 (S38W08 L=322) 334 45 1 (1356/ 417-1384/ 480) 68.2 W06-W09 S40-S35
19 971 242 (S43E30 L=284) 3172 336 6 ( 858/ 125-1043/ 369) 24.9 E58-E17 S52-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20230907 ...
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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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