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| 20260613 - Filament data for 09 UTC |
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Available data for 20260613: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 671 1593 (N32E35 L=268) 1523 252 0 ( 612/1478- 717/1689) -37.4 E45-E28 N24-N37
2 1703 1474 (N38W51 L=354) 600 81 1 (1664/1436-1728/1495) -36.9 W46-W54 N35-N40
3 1336 1452 (N31W16 L=319) 549 121 1 (1307/1397-1371/1490) 60.3 W13-W18 N27-N34
4 512 1427 (N19E41 L=263) 269 75 0 ( 486/1407- 550/1458) -18.4 E43-E37 N17-N20
5 864 1403 (N22E15 L=288) 407 116 0 ( 820/1363- 923/1428) 39.8 E17-E11 N18-N24
6 1652 1257 (N23W41 L=344) 439 77 1 (1619/1226-1679/1284) -36.9 W38-W43 N20-N24
7 916 1159 (N07E08 L=295) 281 189 0 ( 892/1110- 974/1225) -45.0 E10-E04 N04-N11
8 1333 1172 (N13W17 L=321) 265 95 0 (1303/1129-1355/1215) 63.4 W15-W18 N10-N16
9 1862 1166 (N19W63 L= 7) 474 61 2 (1827/1150-1885/1188) 14.0 W58-W67 N18-N20
10 124 1120 (S05E74 L=229) 991 83 4 ( 108/1081- 143/1165) 90.0 E78-E70 S07-S02
11 324 1112 (S03E48 L=255) 412 78 0 ( 305/1076- 345/1141) -45.0 E50-E46 S04-N00
12 209 836 (S21E60 L=243) 934 137 0 ( 187/ 791- 244/ 907) 76.0 E63-E56 S24-S16
13 418 870 (S16E39 L=265) 250 44 0 ( 395/ 851- 445/ 886) 14.0 E40-E36 S17-S15
14 1469 833 (S05W30 L=334) 531 164 1 (1405/ 800-1534/ 862) 0.0 W26-W35 S07-S03
15 1454 681 (S15W32 L=336) 361 113 0 (1429/ 635-1479/ 724) 80.5 W31-W33 S17-S11
16 838 639 (S25E07 L=296) 365 62 1 ( 813/ 614- 871/ 668) 36.9 E08-E04 S27-S23
17 657 591 (S31E20 L=284) 437 111 0 ( 610/ 575- 716/ 613) 0.0 E23-E15 S32-S29
18 1654 498 (S24W57 L= 1) 606 117 0 (1630/ 471-1690/ 529) 63.4 W54-W62 S25-S21
19 1240 388 (S37W27 L=330) 1459 226 3 (1125/ 361-1347/ 421) 13.2 W17-W35 S39-S34
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Download FITS filament maps as tar archive
» All Filament Data of 20260613 ...
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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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