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| 20231013 - Filament data for 10 UTC |
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Available data for 20231013: »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 1531 1703 (N28W63 L=260) 598 77 0 (1503/1672-1558/1737) 59.0 W60-W66 N25-N30
2 1175 1678 (N39W34 L=231) 554 110 1 (1125/1661-1233/1696) -20.6 W31-W39 N36-N41
3 1388 1603 (N27W43 L=239) 853 194 1 (1294/1585-1477/1626) -38.7 W37-W50 N23-N31
4 997 1604 (N40W18 L=214) 316 71 1 ( 957/1582-1030/1619) -21.8 W15-W20 N38-N41
5 1460 1458 (N17W40 L=236) 754 310 1 (1310/1435-1591/1484) -22.8 W29-W48 N12-N21
6 1657 1379 (N07W50 L=247) 315 64 0 (1634/1351-1674/1405) -76.0 W49-W51 N04-N08
7 1078 1344 (N22W12 L=208) 584 154 1 (1004/1322-1148/1371) -11.3 W07-W17 N20-N24
8 584 1212 (N28E22 L=174) 561 238 0 ( 490/1149- 670/1274) -45.0 E28-E17 N22-N33
9 1865 1029 (S19W58 L=254) 429 64 1 (1842/ 991-1883/1063) 31.0 W54-W61 S20-S17
10 471 1008 (N19E34 L=162) 672 235 2 ( 400/ 976- 591/1042) -23.2 E39-E25 N16-N22
11 358 953 (N18E45 L=152) 333 47 0 ( 327/ 936- 383/ 969) -31.0 E47-E42 N16-N19
12 1769 921 (S22W45 L=242) 330 74 0 (1727/ 909-1809/ 935) -14.0 W41-W49 S23-S19
13 332 813 (N10E50 L=146) 294 41 0 ( 318/ 785- 346/ 841) 56.3 E51-E48 N08-N12
14 1437 762 (S20W17 L=213) 546 252 0 (1368/ 677-1515/ 839) 24.8 W10-W23 S23-S17
15 355 749 (N06E50 L=146) 574 0 -1 ( 309/ 730- 407/ 771) -20.6 E54-E46 N04-N08
16 1140 653 (S18E03 L=193) 279 82 1 (1123/ 625-1169/ 688) -78.7 E04-E02 S20-S15
17 1574 430 (S49W23 L=219) 383 74 0 (1542/ 404-1602/ 460) 18.4 W19-W26 S50-S47
18 494 303 (S24E66 L=130) 758 61 2 ( 472/ 268- 516/ 338) 45.0 E70-E62 S27-S21
19 1345 298 (S51E02 L=194) 783 91 0 (1302/ 272-1393/ 335) 0.0 E06-W03 S53-S48
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Download FITS filament maps as tar archive
» All Filament Data of 20231013 ...
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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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