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| 20241006 - Filament data for 06 UTC |
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Available data for 20241006: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1590 1513 (N16W52 L=192) 457 67 2 (1554/1490-1628/1530) -26.6 W49-W55 N14-N17
2 1730 1431 (N07W59 L=199) 568 98 1 (1683/1402-1759/1467) 0.0 W53-W63 N05-N08
3 1837 1129 (S13W56 L=196) 6286 619 8 (1774/ 865-1925/1325) 37.9 W49-W84 S28-S05
4 1574 1291 (N05W40 L=180) 267 68 0 (1540/1272-1606/1305) -45.0 W37-W42 N02-N06
5 1011 1249 (N19W06 L=145) 498 110 1 ( 947/1232-1077/1267) -20.6 W01-W09 N16-N20
6 849 1152 (N18E06 L=133) 451 198 0 ( 770/1104- 915/1199) -45.0 E10-E03 N13-N21
7 1688 1155 (S06W43 L=183) 399 75 1 (1665/1127-1719/1184) -76.0 W41-W45 S08-S04
8 1887 1154 (S13W64 L=203) 585 63 1 (1863/1115-1904/1184) -90.0 W60-W66 S15-S11
9 277 974 (N21E51 L= 88) 2071 381 3 ( 176/ 835- 362/1145) -52.7 E62-E45 N12-N33
10 1685 1051 (S11W40 L=180) 307 116 1 (1640/1029-1722/1084) -8.1 W36-W43 S12-S09
11 1750 1014 (S16W45 L=184) 767 107 1 (1709/ 959-1779/1058) 68.2 W41-W46 S19-S13
12 963 1024 (N08E03 L=136) 206 107 0 ( 912/1010-1013/1040) -9.5 E06-W00 N07-N09
13 489 976 (N17E33 L=106) 428 151 0 ( 435/ 939- 549/1013) -40.6 E37-E29 N13-N19
14 1224 802 (S11W05 L=145) 882 349 1 (1175/ 641-1249/ 947) 53.7 E02-W09 S19-S03
15 1577 887 (S17W28 L=168) 352 91 0 (1526/ 872-1621/ 898) -26.6 W25-W31 S18-S14
16 1366 561 (S30W07 L=147) 3469 582 8 (1216/ 370-1531/ 780) 28.1 E08-W22 S38-S20
17 1115 673 (S15E05 L=135) 252 114 0 (1059/ 653-1166/ 687) -38.7 E07-E01 S17-S13
18 384 617 (S01E52 L= 88) 1368 200 3 ( 302/ 565- 464/ 681) -21.0 E60-E47 S05-N02
19 556 611 (S05E39 L=101) 951 217 5 ( 508/ 498- 590/ 680) 65.6 E44-E34 S11-N00
20 754 446 (S19E34 L=106) 1114 317 3 ( 732/ 301- 790/ 589) 46.6 E42-E25 S29-S11
21 925 462 (S23E22 L=117) 803 273 2 ( 865/ 364- 960/ 572) 40.2 E30-E16 S28-S16
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Download FITS filament maps as tar archive
» All Filament Data of 20241006 ...
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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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