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| 20241207 - Filament data for 09 UTC |
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Available data for 20241207: »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 1549 1648 (N30W51 L= 92) 1210 153 1 (1521/1573-1580/1723) 57.5 W47-W57 N24-N35
2 1288 1592 (N31W27 L= 68) 694 159 0 (1204/1574-1362/1607) -20.0 W21-W32 N28-N32
3 1689 1520 (N20W57 L= 97) 467 90 1 (1651/1485-1732/1545) -33.7 W53-W59 N17-N21
4 1788 1478 (N16W65 L=106) 566 74 1 (1764/1443-1805/1514) 39.8 W62-W70 N13-N18
5 1860 1357 (N08W68 L=109) 515 69 0 (1839/1327-1875/1396) 26.6 W63-W72 N06-N10
6 732 1217 (N15E15 L= 26) 315 112 0 ( 694/1175- 773/1260) -56.3 E16-E12 N12-N18
7 1312 1053 (S02W17 L= 58) 882 279 3 (1248/ 947-1411/1119) 32.5 W12-W23 S07-N00
8 840 923 (S03E12 L= 29) 1601 410 2 ( 705/ 738- 932/1035) -63.4 E19-E09 S15-N04
9 1458 938 (S11W25 L= 66) 619 202 0 (1430/ 847-1481/1026) 68.2 W22-W27 S15-S05
10 1633 988 (S10W38 L= 79) 646 139 3 (1569/ 950-1698/1026) -12.5 W33-W42 S13-S07
11 717 816 (S08E21 L= 20) 307 119 1 ( 676/ 780- 749/ 857) 21.8 E23-E18 S09-S05
12 186 716 (S06E67 L=334) 1056 90 4 ( 154/ 682- 222/ 754) 4.8 E73-E61 S08-S04
13 427 720 (S10E43 L=358) 249 63 1 ( 399/ 693- 454/ 745) 0.0 E45-E40 S10-S08
14 949 515 (S30E13 L= 28) 2367 488 6 ( 846/ 346-1012/ 740) 53.1 E25-E07 S39-S15
15 1358 659 (S26W16 L= 57) 1188 298 2 (1219/ 608-1479/ 728) 6.0 W06-W25 S28-S23
16 339 680 (S11E51 L=349) 669 113 1 ( 303/ 639- 373/ 712) -59.0 E54-E47 S13-S08
17 446 632 (S15E44 L=357) 1028 190 5 ( 390/ 577- 525/ 691) 4.8 E49-E37 S17-S11
18 414 492 (S23E53 L=348) 2966 363 3 ( 292/ 403- 561/ 606) 10.5 E79-E36 S27-S17
19 703 294 (S41E41 L=360) 637 72 2 ( 665/ 269- 737/ 319) 12.5 E45-E36 S43-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20241207 ...
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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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