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| 20231112 - Filament data for 09 UTC |
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Available data for 20231112: »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 1265 1725 (N39W40 L=201) 1049 207 1 (1167/1675-1361/1760) -2.9 W30-W50 N37-N40
2 1428 1535 (N23W40 L=201) 319 101 0 (1390/1508-1473/1566) -63.4 W37-W41 N19-N25
3 481 1336 (N34E30 L=132) 770 192 0 ( 396/1316- 577/1354) -10.6 E37-E21 N31-N35
4 1107 1266 (N15W10 L=171) 276 89 0 (1059/1246-1148/1281) -31.0 W07-W12 N12-N16
5 1808 1213 (S05W57 L=218) 427 84 0 (1782/1167-1827/1249) -78.7 W55-W58 S07-S02
6 680 1227 (N22E16 L=145) 358 80 0 ( 640/1199- 724/1248) 9.5 E19-E13 N21-N23
7 1739 1048 (S12W46 L=207) 1292 273 2 (1672/ 971-1796/1130) -61.4 W41-W52 S17-S06
8 278 1008 (N18E51 L=111) 1650 326 1 ( 145/ 943- 388/1108) 6.1 E67-E39 N14-N21
9 1839 1026 (S16W56 L=217) 470 65 0 (1820/ 995-1858/1070) 45.0 W53-W59 S18-S14
10 1433 947 (S10W22 L=183) 223 53 0 (1414/ 922-1448/ 980) 45.0 W20-W23 S11-S08
11 1924 913 (S26W68 L=229) 631 50 1 (1903/ 885-1949/ 935) 6.3 W64-W74 S27-S23
12 1560 798 (S22W28 L=189) 347 61 0 (1539/ 766-1577/ 837) 68.2 W26-W29 S24-S19
13 1388 729 (S22W15 L=176) 773 204 0 (1322/ 647-1440/ 817) 32.5 W09-W20 S25-S18
14 1184 664 (S21W01 L=162) 1013 287 0 (1146/ 546-1252/ 804) 52.4 E03-W08 S27-S14
15 870 651 (S15E18 L=143) 301 105 0 ( 840/ 614- 912/ 699) 29.7 E20-E13 S16-S12
16 1412 597 (S31W15 L=176) 515 118 0 (1356/ 568-1460/ 639) 7.1 W10-W18 S32-S29
17 358 582 (S08E56 L=105) 343 32 1 ( 341/ 561- 378/ 604) -45.0 E58-E54 S09-S07
18 824 446 (S26E28 L=133) 553 151 1 ( 787/ 376- 850/ 517) 38.7 E33-E23 S30-S22
19 1630 449 (S50W35 L=196) 957 117 0 (1565/ 426-1687/ 479) -3.6 W27-W43 S52-S48
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Download FITS filament maps as tar archive
» All Filament Data of 20231112 ...
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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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