|
|
|
|
| 20240726 - Latest Filament data |
|
Available data for 20240726: »06 UTC »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 1322 1731 (N49W40 L= 48) 482 67 2 (1292/1698-1346/1759) 78.7 W38-W43 N45-N50
2 1269 1620 (N41W28 L= 35) 482 91 1 (1229/1582-1301/1643) -45.0 W24-W30 N37-N42
3 1599 1605 (N34W58 L= 65) 428 55 1 (1577/1579-1620/1638) 53.1 W55-W60 N32-N36
4 1708 1490 (N25W62 L= 69) 766 108 1 (1664/1451-1746/1521) -45.0 W57-W64 N22-N27
5 354 1425 (N35E52 L=315) 450 73 1 ( 319/1408- 388/1447) -11.3 E57-E47 N34-N36
6 1057 1417 (N29W06 L= 14) 297 121 1 (1000/1391-1108/1443) -29.7 W02-W09 N27-N31
7 1580 1058 (N01W36 L= 44) 228 51 1 (1558/1032-1598/1086) 33.7 W34-W37 N00-N02
8 516 829 (S03E35 L=333) 232 76 0 ( 485/ 799- 540/ 857) -53.1 E36-E33 S04-N00
9 1733 794 (S17W48 L= 56) 467 130 1 (1703/ 750-1752/ 830) 90.0 W45-W50 S20-S14
10 391 720 (S09E47 L=321) 820 188 3 ( 355/ 641- 422/ 792) -84.3 E49-E43 S14-S04
11 1013 702 (S14E04 L= 4) 279 180 0 ( 966/ 677-1070/ 754) -45.0 E06-W00 S16-S10
12 1117 640 (S19W02 L= 10) 522 179 1 (1041/ 602-1157/ 708) 39.8 E02-W04 S21-S15
13 1669 615 (S29W44 L= 52) 825 220 1 (1576/ 582-1763/ 651) -3.0 W35-W54 S30-S27
14 1261 532 (S29W11 L= 19) 1387 423 1 (1122/ 433-1442/ 649) 24.6 W00-W24 S34-S22
15 832 548 (S23E18 L=350) 406 136 0 ( 801/ 493- 884/ 601) 45.0 E20-E13 S26-S19
16 1281 425 (S37W13 L= 20) 538 158 3 (1212/ 405-1366/ 452) 0.0 W07-W19 S38-S35
17 938 293 (S44E17 L=351) 1436 210 2 ( 887/ 217-1015/ 349) 36.9 E24-E08 S51-S39
18 1030 215 (S54E12 L=355) 364 64 0 (1005/ 197-1063/ 236) -51.3 E13-E09 S56-S50
|
Download FITS filament maps as tar archive
» All Filament Data of 20240726 ...
|
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.
|
|
|
|