|
|
|
|
| 20240927 - Latest Filament data |
|
Available data for 20240927: »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1538 1696 (N27W62 L=319) 2019 195 3 (1448/1653-1616/1730) -16.4 W51-W71 N22-N29
2 1379 1452 (N20W34 L=290) 835 222 0 (1256/1413-1464/1483) -11.3 W25-W40 N17-N21
3 1216 1233 (N13W16 L=273) 866 252 0 (1161/1123-1274/1333) -90.0 W14-W17 N05-N19
4 480 1222 (N32E30 L=226) 753 156 2 ( 418/1183- 546/1254) -20.0 E35-E24 N28-N34
5 1869 1096 (S15W59 L=315) 407 58 0 (1855/1062-1885/1124) 71.6 W57-W61 S16-S13
6 222 857 (N15E60 L=196) 851 105 4 ( 197/ 794- 248/ 904) 81.9 E62-E57 N11-N18
7 830 817 (N00E16 L=240) 593 184 2 ( 790/ 743- 877/ 901) 29.1 E20-E11 S03-N04
8 1688 865 (S21W37 L=293) 661 84 1 (1651/ 819-1722/ 901) 26.6 W33-W39 S23-S18
9 1290 770 (S14W08 L=264) 593 208 1 (1198/ 731-1374/ 797) -9.5 W01-W13 S16-S12
10 622 723 (S00E31 L=225) 225 47 1 ( 596/ 701- 644/ 747) -45.0 E32-E29 S01-N01
11 1605 676 (S30W27 L=283) 436 53 1 (1575/ 642-1631/ 706) 36.9 W24-W29 S32-S28
12 484 453 (S13E52 L=204) 3273 532 4 ( 425/ 236- 531/ 699) 45.0 E75-E43 S29-N02
13 1317 653 (S22W07 L=263) 274 105 0 (1269/ 620-1350/ 696) 18.4 W03-W09 S23-S20
14 684 507 (S14E35 L=221) 530 117 1 ( 647/ 462- 718/ 563) 82.9 E36-E33 S17-S09
15 808 502 (S17E27 L=229) 289 108 0 ( 766/ 463- 845/ 543) 20.6 E31-E23 S18-S15
16 370 443 (S12E64 L=192) 1576 99 2 ( 323/ 403- 413/ 482) -50.2 E69-E60 S14-S08
17 1459 457 (S40W12 L=268) 286 31 0 (1440/ 434-1476/ 478) 71.6 W10-W13 S42-S38
18 1341 346 (S45E01 L=256) 1246 227 0 (1247/ 283-1416/ 406) 13.2 E10-W07 S47-S41
19 680 211 (S34E57 L=199) 1093 93 1 ( 638/ 181- 715/ 246) 11.3 E66-E50 S36-S32
|
Download FITS filament maps as tar archive
» All Filament Data of 20240927 ...
|
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.
|
|
|
|