|
|
|
|
| 20250702 - Filament data for 10 UTC |
|
Available data for 20250702: »05 UTC »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 1591 1680 (N48W59 L=247) 564 63 0 (1560/1658-1619/1702) 7.6 W51-W66 N45-N49
2 1206 1546 (N37W12 L=201) 298 99 1 (1166/1523-1239/1569) 9.5 W09-W15 N35-N38
3 301 1523 (N31E67 L=121) 622 60 1 ( 275/1504- 333/1546) -4.4 E75-E62 N30-N32
4 1263 1488 (N33W16 L=205) 266 24 0 (1241/1467-1286/1511) 0.0 W14-W17 N31-N34
5 485 1471 (N29E43 L=146) 1017 227 4 ( 403/1441- 607/1508) -3.0 E50-E31 N26-N31
6 1285 1329 (N22W17 L=205) 261 86 0 (1274/1290-1299/1375) 71.6 W15-W17 N19-N25
7 301 1154 (N08E51 L=137) 581 138 0 ( 281/1098- 329/1221) -53.1 E54-E48 N04-N12
8 1658 1144 (N11W43 L=232) 423 96 0 (1616/1106-1693/1175) -33.7 W39-W45 N08-N12
9 625 1074 (N05E25 L=163) 246 109 0 ( 594/1027- 669/1102) 45.0 E27-E22 N01-N06
10 1713 982 (N01W47 L=236) 922 181 1 (1680/ 908-1737/1056) -76.0 W44-W49 S03-N05
11 1600 751 (S13W40 L=228) 346 66 0 (1576/ 721-1624/ 778) -31.0 W37-W42 S15-S11
12 276 696 (S21E57 L=132) 664 130 0 ( 222/ 666- 319/ 736) 23.2 E65-E50 S23-S17
13 1765 583 (S25W62 L=251) 2260 212 2 (1685/ 517-1818/ 665) 45.0 W54-W69 S29-S19
14 886 580 (S25E08 L=180) 804 227 0 ( 822/ 544- 971/ 639) -16.7 E12-E02 S27-S21
15 670 577 (S27E24 L=165) 294 79 0 ( 629/ 557- 708/ 602) 26.6 E26-E20 S28-S24
16 1372 235 (S53W42 L=231) 737 93 1 (1336/ 214-1407/ 263) -17.4 W34-W50 S55-S50
17 1285 216 (S56W33 L=222) 567 55 1 (1266/ 188-1301/ 245) -31.0 W28-W38 S59-S52
18 1230 203 (S57W27 L=216) 565 60 2 (1191/ 182-1262/ 221) 0.0 W22-W31 S59-S54
|
Download FITS filament maps as tar archive
» All Filament Data of 20250702 ...
|
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.
|
|
|
|