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| 20251110 - Filament data for 07 UTC |
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Available data for 20251110: »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 1353 1855 (N44W63 L=323) 1417 100 1 (1321/1817-1384/1899) 7.1 W54-W78 N42-N46
2 1249 1825 (N46W48 L=309) 597 62 1 (1223/1789-1274/1856) 15.3 W43-W54 N43-N47
3 1279 1631 (N32W34 L=295) 774 114 0 (1219/1600-1335/1660) -50.2 W31-W37 N28-N35
4 977 1527 (N34W10 L=270) 535 209 0 ( 955/1435- 999/1623) 69.0 W07-W13 N27-N40
5 1059 1558 (N33W16 L=277) 299 68 1 (1039/1512-1082/1587) 38.7 W13-W18 N30-N35
6 1675 1470 (N12W55 L=315) 2137 226 2 (1582/1410-1781/1542) -39.8 W49-W63 N07-N18
7 403 1520 (N48E38 L=222) 567 66 0 ( 371/1497- 440/1541) -6.3 E42-E33 N46-N50
8 1242 1463 (N23W24 L=284) 277 90 0 (1202/1440-1278/1481) -45.0 W21-W25 N21-N24
9 716 1383 (N31E11 L=249) 975 246 1 ( 585/1365- 830/1400) -16.4 E20-E03 N28-N34
10 1193 1320 (N16W17 L=277) 519 230 0 (1115/1261-1290/1371) 8.7 W10-W23 N14-N17
11 1036 1301 (N19W07 L=267) 207 106 0 ( 997/1274-1084/1324) -45.0 W05-W09 N16-N20
12 960 1096 (N09E02 L=258) 953 343 1 ( 840/1064-1146/1133) -13.2 E09-W08 N04-N11
13 1631 1047 (S09W37 L=297) 854 135 0 (1590/ 986-1675/1113) -66.0 W35-W39 S13-S04
14 1807 1027 (S15W52 L=312) 423 57 1 (1788/ 997-1825/1060) 36.9 W49-W53 S16-S13
15 219 927 (N14E57 L=203) 1244 211 1 ( 150/ 835- 281/ 998) -47.7 E65-E52 N08-N19
16 395 766 (N02E45 L=215) 377 96 0 ( 368/ 736- 432/ 789) -9.5 E47-E41 N00-N03
17 854 685 (S12E18 L=243) 822 147 3 ( 797/ 612- 899/ 752) 83.7 E20-E15 S16-S07
18 1498 586 (S34W20 L=281) 696 127 1 (1440/ 553-1554/ 626) 0.0 W15-W25 S35-S32
19 476 463 (S17E51 L=209) 1787 294 6 ( 410/ 365- 543/ 555) 81.9 E56-E47 S24-S10
20 540 332 (S27E55 L=205) 1004 160 1 ( 467/ 297- 588/ 392) 13.2 E65-E48 S29-S23
21 866 199 (S45E41 L=219) 1591 158 1 ( 796/ 157- 922/ 257) 14.7 E51-E32 S48-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20251110 ...
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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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