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| 20260620 - Filament data for 09 UTC |
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Available data for 20260620: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1495 1665 (N50W38 L=248) 687 58 1 (1468/1632-1526/1700) -90.0 W35-W41 N46-N52
2 1237 1394 (N27W11 L=222) 971 246 0 (1185/1286-1288/1497) -60.3 W06-W14 N19-N33
3 546 1397 (N20E36 L=174) 518 164 0 ( 490/1365- 629/1439) -13.0 E42-E29 N18-N21
4 981 1381 (N23E06 L=204) 297 94 0 ( 942/1343-1010/1415) -38.7 E09-E04 N20-N25
5 711 1300 (N15E23 L=188) 312 114 0 ( 686/1250- 731/1348) -63.4 E25-E21 N12-N18
6 608 1219 (N09E28 L=183) 212 59 0 ( 584/1192- 634/1247) 63.4 E29-E26 N07-N11
7 1876 1089 (N12W65 L=276) 1143 156 1 (1840/1009-1904/1157) -66.0 W60-W69 N07-N16
8 129 1026 (S07E72 L=139) 1450 98 5 ( 97/ 966- 154/1070) 90.0 E80-E67 S11-S04
9 1208 1030 (N04W11 L=222) 766 268 1 (1104/ 973-1298/1067) 4.8 W05-W17 N00-N06
10 938 934 (S05E04 L=206) 501 119 1 ( 898/ 889- 992/ 981) -29.7 E07-W00 S06-S02
11 1711 924 (N01W48 L=258) 392 62 0 (1697/ 889-1727/ 959) 71.6 W46-W48 N00-N03
12 675 875 (S11E20 L=190) 660 160 0 ( 605/ 850- 757/ 893) 5.7 E25-E15 S12-S08
13 1752 626 (S17W60 L=271) 1427 164 1 (1694/ 572-1799/ 703) 60.9 W54-W63 S20-S11
14 1453 641 (S18W32 L=243) 282 105 0 (1427/ 594-1489/ 683) 63.4 W31-W34 S21-S15
15 1487 600 (S21W36 L=247) 310 94 0 (1442/ 577-1520/ 632) 45.0 W33-W38 S22-S18
16 1417 493 (S28W34 L=245) 301 39 0 (1394/ 472-1444/ 518) -11.3 W32-W37 S29-S26
17 1566 495 (S27W47 L=258) 420 60 0 (1544/ 477-1604/ 514) 11.3 W44-W50 S28-S25
18 798 463 (S37E11 L=200) 2067 417 3 ( 614/ 427-1004/ 498) 7.6 E26-W04 S41-S32
19 359 438 (S45E60 L=151) 609 70 1 ( 328/ 424- 397/ 463) 0.0 E66-E53 S46-S43
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Download FITS filament maps as tar archive
» All Filament Data of 20260620 ...
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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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