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| 20260618 - Filament data for 09 UTC |
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Available data for 20260618: »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 1295 1652 (N46W15 L=252) 414 61 0 (1275/1613-1311/1681) -80.5 W12-W16 N42-N48
2 854 1422 (N24E16 L=221) 599 204 0 ( 817/1335- 899/1512) -48.0 E20-E11 N18-N29
3 1629 1464 (N35W43 L=280) 1233 132 5 (1561/1430-1685/1504) 4.4 W35-W48 N33-N38
4 617 1434 (N22E32 L=205) 263 88 2 ( 593/1390- 633/1472) -45.0 E35-E30 N19-N24
5 231 1378 (N14E67 L=170) 739 125 0 ( 212/1321- 255/1439) -69.4 E70-E63 N10-N18
6 345 1410 (N18E55 L=182) 463 101 1 ( 297/1373- 393/1436) -8.7 E61-E48 N15-N18
7 984 1142 (N08E04 L=234) 227 99 0 ( 937/1114-1027/1182) -18.4 E06-W00 N06-N10
8 1587 1141 (N14W36 L=273) 320 84 1 (1570/1094-1599/1177) 90.0 W34-W36 N10-N16
9 783 1092 (N03E15 L=222) 726 256 1 ( 677/1044- 878/1119) 4.8 E21-E09 N00-N05
10 508 1010 (S05E33 L=205) 684 130 4 ( 464/ 954- 546/1067) -50.2 E36-E29 S07-S01
11 1841 1015 (N08W60 L=297) 397 99 0 (1817/ 985-1876/1056) -29.7 W57-W64 N06-N10
12 315 954 (S10E48 L=189) 743 146 2 ( 253/ 928- 387/ 997) 17.1 E54-E41 S12-S06
13 772 836 (S13E14 L=223) 459 141 0 ( 718/ 804- 830/ 885) -23.2 E17-E09 S14-S09
14 1079 664 (S20W07 L=244) 462 237 1 (1049/ 616-1137/ 749) -83.7 W05-W11 S23-S14
15 514 696 (S24E32 L=206) 345 102 0 ( 484/ 670- 563/ 736) -18.4 E33-E27 S25-S21
16 1445 671 (S16W31 L=269) 532 127 0 (1391/ 628-1493/ 726) 54.5 W28-W33 S19-S12
17 1052 549 (S28W07 L=244) 214 57 0 (1023/ 531-1084/ 571) -14.0 W05-W09 S29-S26
18 1238 536 (S27W20 L=257) 269 39 1 (1225/ 509-1256/ 568) -76.0 W18-W21 S28-S24
19 454 515 (S38E40 L=197) 2653 400 8 ( 297/ 468- 646/ 563) 7.9 E67-E22 S44-S33
20 1554 441 (S30W50 L=287) 681 94 2 (1503/ 425-1605/ 462) 5.7 W44-W54 S31-S28
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Download FITS filament maps as tar archive
» All Filament Data of 20260618 ...
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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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