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| 20240518 - Filament data for 10 UTC |
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Available data for 20240518: »05 UTC »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
1 649 1791 (N38E57 L=145) 1244 147 3 ( 597/1747- 705/1842) -7.9 E76-E47 N35-N41
2 623 1675 (N29E48 L=155) 1074 192 2 ( 532/1637- 705/1723) 42.0 E53-E43 N24-N33
3 1449 1536 (N40W18 L=220) 1223 227 3 (1369/1448-1490/1610) -39.3 W10-W21 N33-N45
4 339 1540 (N14E66 L=137) 679 78 1 ( 315/1498- 368/1576) -68.2 E67-E63 N11-N16
5 906 1518 (N25E20 L=182) 401 189 0 ( 846/1445- 964/1574) -22.6 E25-E13 N21-N27
6 1355 1411 (N29W12 L=214) 1408 496 1 (1210/1211-1442/1553) -37.3 W00-W21 N17-N35
7 939 1345 (N15E12 L=190) 862 299 4 ( 811/1303-1066/1393) 3.2 E21-E03 N12-N17
8 1703 1210 (N25W42 L=244) 892 176 2 (1676/1134-1734/1270) -49.4 W39-W45 N20-N28
9 1776 1222 (N27W50 L=252) 379 93 0 (1737/1190-1810/1241) -7.1 W45-W54 N26-N28
10 240 1198 (S08E60 L=143) 380 46 0 ( 222/1172- 259/1221) -45.0 E61-E57 S09-S06
11 224 1139 (S12E60 L=142) 1777 213 4 ( 153/1055- 304/1200) 50.7 E69-E52 S17-S06
12 1899 1015 (N18W68 L=270) 932 120 0 (1883/ 958-1912/1076) -54.5 W64-W71 N14-N21
13 246 1019 (S19E55 L=147) 485 41 1 ( 224/ 989- 266/1046) -71.6 E57-E53 S20-S17
14 371 958 (S20E42 L=160) 732 193 1 ( 309/ 893- 411/1040) 63.4 E47-E39 S24-S14
15 1286 786 (S10W21 L=223) 248 55 2 (1258/ 757-1312/ 813) -14.0 W18-W22 S11-S08
16 1127 683 (S20W14 L=216) 572 214 1 (1027/ 660-1218/ 705) 32.5 W08-W19 S23-S16
17 509 625 (S38E28 L=174) 1998 352 6 ( 363/ 569- 646/ 702) -2.1 E42-E15 S41-S35
18 295 663 (S41E52 L=150) 1212 125 2 ( 234/ 643- 355/ 697) 11.9 E63-E44 S43-S38
19 513 470 (S51E28 L=174) 347 62 1 ( 486/ 453- 541/ 490) 0.0 E31-E25 S51-S48
20 1230 349 (S39W36 L=238) 530 100 1 (1208/ 322-1266/ 394) -20.6 W31-W39 S40-S35
21 831 354 (S50W05 L=207) 327 87 0 ( 797/ 334- 876/ 377) -6.3 W01-W10 S51-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20240518 ...
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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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