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| 20251111 - Filament data for 14 UTC |
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Available data for 20251111: »07 UTC »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 1453 1696 (N31W51 L=295) 431 61 2 (1413/1672-1481/1715) -53.1 W48-W53 N29-N33
2 1203 1555 (N29W25 L=269) 267 59 0 (1181/1528-1220/1594) 45.0 W23-W27 N27-N31
3 554 1564 (N47E22 L=222) 330 44 1 ( 526/1545- 584/1581) -18.4 E24-E18 N46-N48
4 1439 1553 (N23W41 L=284) 364 82 2 (1405/1531-1480/1579) -53.1 W38-W42 N21-N25
5 416 1534 (N49E37 L=206) 556 81 1 ( 388/1491- 442/1569) 80.5 E40-E33 N45-N51
6 1346 1534 (N25W34 L=277) 345 91 2 (1315/1487-1370/1569) 51.3 W31-W35 N21-N26
7 939 1477 (N31W06 L=249) 1168 334 3 ( 776/1450-1098/1497) -15.9 E05-W16 N27-N34
8 1443 1435 (N17W36 L=279) 485 191 0 (1370/1393-1508/1489) 8.7 W29-W42 N15-N18
9 1238 1209 (N09W16 L=260) 1178 319 3 (1107/1171-1385/1254) -13.2 W07-W24 N04-N11
10 360 1017 (N16E42 L=201) 936 219 4 ( 274/ 943- 443/1064) -34.7 E49-E36 N10-N19
11 1105 812 (S10E00 L=243) 253 70 2 (1086/ 776-1125/ 854) 63.4 E01-W01 S12-S08
12 1682 665 (S34W37 L=280) 633 110 0 (1625/ 638-1730/ 701) 0.0 W31-W42 S35-S32
13 670 615 (S12E31 L=213) 269 93 0 ( 619/ 602- 710/ 637) 8.1 E34-E27 S13-S11
14 552 587 (S12E39 L=204) 251 64 0 ( 532/ 554- 575/ 621) 63.4 E40-E37 S13-S09
15 664 498 (S19E35 L=208) 311 42 1 ( 643/ 466- 684/ 524) 63.4 E36-E33 S21-S17
16 358 473 (S15E62 L=182) 594 119 2 ( 307/ 445- 406/ 504) -18.4 E66-E56 S17-S12
17 689 443 (S23E36 L=207) 267 97 0 ( 645/ 429- 723/ 476) 0.0 E39-E32 S24-S21
18 539 332 (S27E55 L=188) 1559 174 3 ( 468/ 288- 626/ 366) 2.6 E67-E45 S29-S24
19 996 248 (S45E27 L=217) 1489 202 3 ( 909/ 201-1082/ 308) 0.0 E35-E17 S47-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20251111 ...
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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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