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| 20241110 - Filament data for 09 UTC |
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Available data for 20241110: »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 1340 1639 (N30W39 L= 76) 1261 244 2 (1233/1584-1452/1674) -2.9 W29-W49 N28-N31
2 1672 1620 (N20W65 L=102) 1572 185 1 (1599/1563-1743/1673) -55.0 W60-W71 N14-N24
3 1576 1583 (N21W53 L= 90) 2154 342 5 (1413/1487-1711/1639) -50.5 W43-W60 N11-N28
4 1353 1492 (N21W32 L= 69) 261 108 0 (1298/1481-1404/1503) -23.2 W28-W35 N19-N22
5 1724 1110 (S09W45 L= 82) 1258 305 2 (1661/1034-1767/1224) 70.0 W39-W49 S12-S01
6 422 1123 (N22E36 L= 1) 701 168 1 ( 342/1067- 469/1159) -41.6 E41-E32 N17-N25
7 1407 957 (S09W20 L= 57) 279 119 0 (1386/ 905-1425/1009) 68.2 W18-W21 S11-S06
8 868 868 (S02E12 L= 25) 1798 441 7 ( 724/ 694- 964/ 980) -70.6 E19-E09 S13-N05
9 1335 924 (S09W15 L= 52) 431 102 2 (1299/ 884-1358/ 975) 45.0 W12-W17 S11-S06
10 1189 892 (S08W06 L= 43) 427 156 2 (1153/ 833-1210/ 950) 56.3 W02-W08 S10-S03
11 348 899 (N11E45 L=351) 699 158 2 ( 287/ 865- 425/ 945) -31.0 E49-E39 N07-N14
12 1241 916 (S08W10 L= 46) 251 36 1 (1219/ 888-1264/ 941) 45.0 W08-W11 S09-S06
13 1442 662 (S28W17 L= 54) 1288 249 6 (1334/ 625-1544/ 713) -11.3 W09-W24 S29-S24
14 559 669 (S06E36 L= 1) 305 38 0 ( 536/ 641- 581/ 690) -90.0 E37-E34 S08-S04
15 1130 406 (S36E10 L= 27) 3582 665 7 ( 969/ 185-1228/ 681) 42.3 E34-W00 S49-S18
16 542 591 (S10E40 L=357) 703 110 3 ( 486/ 554- 581/ 626) -45.0 E43-E37 S13-S08
17 527 422 (S20E50 L=347) 2778 467 4 ( 384/ 317- 629/ 564) 14.3 E79-E36 S24-S13
18 1045 329 (S39E19 L= 18) 292 72 0 (1031/ 290-1057/ 369) 50.2 E21-E16 S42-S36
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Download FITS filament maps as tar archive
» All Filament Data of 20241110 ...
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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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