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| 20231219 - Filament data for 10 UTC |
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Available data for 20231219: »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
1 652 1527 (N33E22 L= 11) 4581 685 12 ( 401/1321- 890/1669) -31.1 E53-E05 N17-N46
2 1355 1618 (N33W30 L= 63) 460 155 1 (1284/1595-1421/1645) -24.0 W25-W34 N31-N35
3 1161 1488 (N26W13 L= 46) 772 310 1 (1060/1399-1291/1587) -45.0 W07-W20 N19-N33
4 1679 1517 (N24W55 L= 87) 372 47 1 (1658/1496-1706/1533) 9.5 W52-W58 N22-N25
5 345 1457 (N32E49 L=344) 415 65 0 ( 318/1432- 378/1480) 33.7 E52-E45 N30-N33
6 435 1415 (N28E39 L=354) 451 130 1 ( 385/1368- 469/1457) -49.4 E44-E35 N24-N31
7 394 1308 (N21E41 L=352) 752 205 1 ( 369/1254- 441/1399) -63.4 E43-E36 N17-N27
8 240 1269 (N20E56 L=337) 992 150 2 ( 211/1199- 276/1331) 66.8 E59-E52 N16-N24
9 183 1208 (N17E62 L=331) 838 138 2 ( 165/1135- 204/1260) -82.9 E65-E59 N12-N20
10 479 1159 (N11E34 L=359) 575 255 1 ( 407/1075- 567/1229) 26.6 E39-E27 N06-N15
11 311 1200 (N15E48 L=345) 423 69 1 ( 280/1175- 349/1223) -26.6 E50-E44 N13-N16
12 329 1113 (N10E46 L=347) 598 122 2 ( 286/1092- 398/1151) -16.7 E49-E39 N08-N12
13 146 1076 (N09E66 L=327) 2366 228 8 ( 92/ 978- 230/1130) 33.7 E77-E55 N03-N13
14 777 751 (S16E18 L= 15) 737 316 1 ( 686/ 647- 872/ 853) 33.7 E25-E10 S21-S10
15 500 723 (S15E37 L=356) 1380 263 3 ( 474/ 592- 531/ 842) 72.6 E40-E33 S23-S07
16 1469 730 (S23W27 L= 60) 1138 280 3 (1368/ 679-1583/ 823) -31.0 W19-W36 S26-S16
17 1657 790 (S20W41 L= 74) 552 138 1 (1598/ 770-1732/ 807) 4.8 W36-W48 S21-S19
18 1675 479 (S42W53 L= 86) 611 74 0 (1645/ 451-1709/ 515) -21.0 W47-W60 S43-S38
19 356 449 (S31E64 L=329) 704 66 0 ( 339/ 408- 374/ 480) 29.1 E68-E59 S33-S28
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Download FITS filament maps as tar archive
» All Filament Data of 20231219 ...
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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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