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| 20230928 - Filament data for 09 UTC |
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Available data for 20230928: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1022 1777 (N52W33 L= 68) 402 52 2 ( 995/1751-1048/1800) 76.0 W30-W35 N50-N54
2 1174 1758 (N45W42 L= 77) 822 80 1 (1139/1730-1221/1783) -7.1 W36-W45 N42-N47
3 1691 1530 (N14W63 L= 98) 809 118 1 (1635/1512-1743/1555) -12.1 W56-W71 N12-N15
4 1118 1365 (N23W15 L= 50) 394 99 1 (1081/1335-1149/1406) 11.3 W12-W17 N21-N25
5 1774 1305 (S00W58 L= 92) 716 125 1 (1744/1241-1794/1365) 63.4 W55-W60 S03-N03
6 902 1331 (N27W01 L= 36) 196 50 0 ( 886/1304- 922/1354) 56.3 W00-W03 N25-N28
7 844 1152 (N18E07 L= 28) 626 179 2 ( 786/1089- 902/1221) 21.8 E11-E01 N16-N21
8 1192 1133 (N08W12 L= 47) 279 73 1 (1165/1107-1214/1167) 33.7 W10-W13 N07-N09
9 289 993 (N22E51 L=344) 2381 516 8 ( 239/ 742- 365/1155) -85.8 E55-E46 N05-N32
10 483 1053 (N21E33 L= 2) 818 231 2 ( 383/ 970- 545/1096) -45.0 E40-E29 N15-N25
11 1867 941 (S24W58 L= 92) 754 113 0 (1832/ 895-1888/ 994) 24.0 W52-W61 S26-S20
12 1567 855 (S18W28 L= 63) 1297 433 2 (1382/ 824-1751/ 914) -14.0 W15-W43 S22-S12
13 1129 757 (S11E01 L= 34) 265 85 0 (1105/ 720-1148/ 794) 45.0 E03-W00 S12-S09
14 1840 770 (S34W54 L= 88) 585 67 1 (1806/ 752-1880/ 787) -22.6 W48-W61 S36-S31
15 1037 577 (S19E12 L= 23) 313 115 1 (1026/ 505-1051/ 632) 63.4 E13-E09 S23-S15
16 689 513 (S14E35 L=360) 800 240 0 ( 648/ 414- 731/ 604) 35.5 E42-E28 S19-S09
17 488 339 (S22E62 L=332) 1924 146 7 ( 445/ 290- 533/ 402) 81.9 E71-E55 S25-S17
18 574 332 (S24E54 L=340) 491 98 0 ( 530/ 312- 600/ 360) 0.0 E57-E49 S25-S22
19 771 309 (S30E41 L=354) 692 104 1 ( 732/ 260- 815/ 348) 24.4 E46-E35 S33-S27
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Download FITS filament maps as tar archive
» All Filament Data of 20230928 ...
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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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