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| 20240910 - Filament data for 09 UTC |
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Available data for 20240910: »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 1145 1744 (N46W37 L=158) 301 44 1 (1129/1715-1164/1773) 38.7 W34-W39 N44-N48
2 1395 1582 (N28W42 L=163) 1041 197 1 (1319/1523-1484/1627) 0.0 W33-W50 N26-N29
3 1518 1431 (N16W42 L=164) 515 177 1 (1456/1389-1596/1468) -4.4 W36-W49 N15-N17
4 1077 1359 (N25W12 L=133) 751 169 4 (1017/1311-1156/1390) -6.3 W07-W16 N22-N26
5 788 1238 (N25E09 L=113) 192 64 0 ( 762/1214- 815/1259) 0.0 E10-E06 N23-N25
6 1787 1032 (S13W50 L=171) 4697 807 14 (1599/ 829-1886/1245) 18.9 W30-W68 S20-S03
7 1056 1170 (N15W05 L=127) 237 122 0 (1016/1121-1083/1214) -81.9 W04-W06 N11-N18
8 1183 1109 (N08W11 L=132) 244 111 0 (1151/1060-1218/1159) 26.6 W08-W14 N06-N10
9 854 1038 (N12E09 L=112) 253 100 0 ( 805/1022- 889/1062) -26.6 E11-E07 N10-N13
10 563 974 (N14E29 L= 93) 422 83 1 ( 527/ 951- 609/1008) -31.0 E31-E26 N12-N16
11 785 899 (N06E16 L=105) 316 114 2 ( 766/ 837- 805/ 951) 71.6 E18-E15 N02-N08
12 852 758 (S04E16 L=105) 516 187 2 ( 782/ 709- 942/ 801) -53.1 E19-E12 S08-N00
13 1811 740 (S32W50 L=171) 616 114 0 (1759/ 715-1851/ 774) 4.8 W43-W55 S33-S31
14 1527 686 (S26W23 L=144) 574 105 2 (1488/ 653-1561/ 723) -71.6 W20-W25 S28-S22
15 1515 551 (S35W20 L=141) 1385 360 0 (1404/ 437-1611/ 701) 31.0 W09-W29 S39-S27
16 1180 566 (S23E02 L=119) 465 177 0 (1113/ 518-1233/ 631) 24.0 E07-W02 S24-S20
17 1669 486 (S46W36 L=157) 971 114 1 (1621/ 447-1712/ 531) 5.7 W29-W40 S49-S42
18 992 425 (S28E18 L=103) 372 115 0 ( 963/ 401-1038/ 474) -80.5 E19-E15 S29-S23
19 434 398 (S18E61 L= 61) 443 49 0 ( 420/ 368- 446/ 428) 45.0 E63-E58 S20-S15
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Download FITS filament maps as tar archive
» All Filament Data of 20240910 ...
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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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