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| 20250407 - Filament data for 09 UTC |
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Available data for 20250407: »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 1300 1786 (N51E09 L=238) 697 87 0 (1258/1761-1344/1810) 7.1 E12-E04 N49-N53
2 404 1627 (N13E62 L=184) 978 93 1 ( 366/1593- 438/1661) 59.0 E66-E59 N10-N15
3 275 1431 (S01E63 L=184) 601 85 0 ( 247/1388- 297/1459) -18.4 E67-E58 S03-N00
4 1673 1436 (N38W32 L=279) 403 23 0 (1651/1416-1694/1455) 0.0 W29-W34 N36-N40
5 228 1328 (S08E64 L=183) 670 90 2 ( 207/1287- 247/1372) 90.0 E66-E61 S10-S04
6 309 1227 (S12E52 L=195) 397 134 1 ( 241/1195- 345/1249) 0.0 E58-E47 S13-S11
7 1330 1186 (N11W12 L=259) 525 110 2 (1281/1139-1372/1239) -18.4 W08-W15 N08-N13
8 650 1171 (S08E25 L=222) 609 200 1 ( 615/1091- 718/1232) 84.3 E26-E22 S12-S02
9 137 1171 (S18E72 L=175) 1892 119 4 ( 90/1129- 205/1198) 10.8 E82-E61 S20-S15
10 990 1089 (S04E04 L=243) 243 77 0 ( 962/1064-1011/1120) 90.0 E04-E02 S05-S01
11 457 957 (S24E33 L=213) 789 211 0 ( 409/ 869- 537/1024) 61.4 E36-E28 S30-S18
12 1267 781 (S12W20 L=267) 272 142 0 (1205/ 760-1337/ 807) 39.8 W17-W23 S15-S09
13 1389 663 (S15W32 L=279) 338 83 0 (1348/ 636-1409/ 699) 78.7 W30-W33 S17-S12
14 535 540 (S49E21 L=226) 1281 276 2 ( 413/ 510- 654/ 600) 6.8 E34-E09 S51-S45
15 1652 554 (S12W56 L=303) 463 103 1 (1626/ 508-1681/ 597) -29.7 W51-W58 S14-S09
16 1219 522 (S28W28 L=275) 481 119 1 (1160/ 501-1284/ 546) 20.6 W23-W31 S29-S25
17 1582 408 (S22W61 L=308) 1228 136 4 (1523/ 355-1638/ 448) 69.4 W57-W64 S26-S18
18 1462 412 (S26W51 L=297) 485 53 1 (1433/ 391-1498/ 435) 18.4 W48-W54 S27-S24
19 1075 275 (S48W36 L=283) 1329 274 0 ( 950/ 214-1178/ 338) 2.0 W22-W50 S49-S46
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Download FITS filament maps as tar archive
» All Filament Data of 20250407 ...
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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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