|
|
|
|
| 20250222 - Filament data for 12 UTC |
|
Available data for 20250222: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1048 1717 (N36E16 L= 89) 617 105 1 ( 999/1684-1099/1740) -6.3 E20-E11 N34-N37
2 391 1535 (N12E54 L= 51) 884 164 3 ( 359/1456- 426/1599) -73.3 E57-E52 N06-N16
3 1246 1507 (N26W03 L=108) 371 100 1 (1207/1465-1286/1554) 66.8 W01-W04 N22-N30
4 1508 1507 (N33W21 L=126) 1603 426 1 (1300/1443-1659/1546) 7.9 W05-W34 N29-N37
5 1092 1255 (N07E01 L=104) 289 92 0 (1048/1234-1140/1275) 36.9 E03-W01 N05-N09
6 203 1212 (S10E62 L= 44) 508 125 0 ( 175/1161- 241/1255) 50.2 E64-E58 S12-S06
7 328 1135 (S13E47 L= 58) 494 128 1 ( 267/1108- 386/1157) 0.0 E52-E41 S13-S11
8 1832 1092 (N16W53 L=158) 770 107 0 (1786/1048-1869/1134) -18.4 W47-W57 N14-N17
9 258 1087 (S16E53 L= 52) 327 65 0 ( 244/1046- 273/1121) 90.0 E54-E51 S18-S14
10 1447 1036 (N03W24 L=129) 192 98 0 (1436/ 986-1462/1083) -68.2 W22-W25 N00-N05
11 1017 1012 (S08E00 L=105) 428 209 0 ( 946/ 960-1100/1047) 40.6 E03-W04 S12-S05
12 1863 875 (N05W61 L=166) 1146 245 0 (1835/ 759-1879/ 984) -67.4 W56-W64 S01-N11
13 317 953 (S24E46 L= 59) 398 72 2 ( 276/ 927- 354/ 977) 14.0 E50-E42 S25-S21
14 776 928 (S17E13 L= 93) 390 196 0 ( 697/ 889- 863/ 965) 33.7 E16-E07 S20-S14
15 1145 836 (S15W11 L=116) 183 59 1 (1124/ 809-1167/ 862) 71.6 W10-W11 S16-S13
16 1303 721 (S18W23 L=128) 245 43 1 (1280/ 697-1330/ 744) 56.3 W21-W24 S19-S16
17 1153 681 (S24W16 L=121) 334 153 0 (1083/ 662-1215/ 716) 6.3 W10-W19 S24-S21
18 1802 599 (S11W67 L=173) 618 70 3 (1776/ 566-1823/ 630) -36.9 W63-W71 S12-S09
|
Download FITS filament maps as tar archive
» All Filament Data of 20250222 ...
|
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.
|
|
|
|