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| 20230928 - Filament data for 08 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 1023 1776 (N52W33 L= 68) 365 45 2 ( 999/1748-1043/1800) 26.6 W30-W36 N50-N54
2 1171 1755 (N45W41 L= 77) 795 92 1 (1134/1727-1221/1779) -33.7 W36-W45 N42-N47
3 1694 1527 (N14W64 L= 99) 709 110 0 (1635/1512-1743/1545) -12.1 W56-W70 N11-N15
4 1111 1377 (N24W15 L= 50) 454 150 1 (1070/1331-1153/1443) 24.0 W11-W20 N21-N27
5 1769 1303 (S00W57 L= 92) 642 107 1 (1740/1244-1792/1359) 63.4 W55-W59 S03-N03
6 839 1154 (N19E07 L= 28) 734 194 2 ( 776/1088- 897/1231) 26.6 E12-E02 N16-N21
7 286 981 (N21E52 L=344) 2435 519 9 ( 237/ 737- 357/1154) -85.8 E55-E46 N05-N32
8 1184 1126 (N08W12 L= 47) 238 38 0 (1159/1107-1207/1145) 0.0 W10-W13 N07-N09
9 483 1046 (N21E33 L= 2) 826 249 2 ( 381/ 958- 543/1094) -47.7 E40-E29 N14-N25
10 1863 940 (S24W57 L= 92) 709 121 0 (1828/ 892-1884/ 994) 26.6 W52-W60 S25-S20
11 394 923 (N16E43 L=353) 348 56 2 ( 363/ 895- 414/ 949) 26.6 E45-E40 N14-N17
12 1560 852 (S18W27 L= 63) 1298 427 1 (1378/ 823-1746/ 914) -14.0 W15-W43 S22-S12
13 1122 753 (S11E02 L= 34) 260 74 1 (1101/ 713-1142/ 787) 45.0 E03-W00 S12-S09
14 1836 766 (S34W53 L= 88) 628 68 1 (1801/ 749-1879/ 784) -21.0 W48-W61 S36-S31
15 692 544 (S13E33 L= 2) 1008 367 1 ( 632/ 411- 748/ 698) 38.3 E43-E24 S19-S04
16 495 367 (S20E59 L=336) 417 47 0 ( 477/ 338- 512/ 395) 51.3 E61-E55 S22-S17
17 569 332 (S24E55 L=340) 507 97 0 ( 527/ 311- 595/ 364) 0.0 E58-E50 S25-S21
18 482 324 (S23E65 L=330) 1262 106 3 ( 443/ 290- 529/ 362) -71.6 E70-E61 S25-S19
19 764 305 (S30E41 L=354) 713 115 1 ( 728/ 257- 809/ 347) 22.6 E47-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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