|
|
|
|
| 20230704 - Filament data for 10 UTC |
|
Available data for 20230704: »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
1 534 1646 (N43E48 L= 42) 364 56 0 ( 516/1627- 555/1670) -20.6 E52-E44 N41-N44
2 1416 1570 (N40W31 L=122) 357 41 1 (1391/1544-1443/1594) -36.9 W29-W33 N37-N41
3 300 1516 (N31E69 L= 22) 983 135 3 ( 279/1448- 327/1577) -22.8 E79-E59 N27-N35
4 1681 1452 (N31W53 L=144) 624 110 1 (1639/1409-1717/1487) -38.7 W49-W56 N27-N33
5 1219 1366 (N25W13 L=103) 410 127 1 (1170/1326-1271/1403) 35.5 W09-W16 N22-N27
6 1496 1238 (N17W31 L=122) 999 325 2 (1390/1136-1614/1328) -38.7 W24-W39 N10-N22
7 1855 1226 (N16W67 L=158) 2065 254 3 (1827/1129-1898/1313) -90.0 W61-W72 N09-N21
8 366 1138 (N08E46 L= 45) 424 200 0 ( 308/1057- 393/1186) -48.8 E51-E43 N02-N10
9 1750 855 (S07W52 L=143) 528 41 1 (1729/ 828-1775/ 880) 71.6 W50-W54 S08-S05
10 905 738 (S15E07 L= 84) 1267 317 4 ( 849/ 617- 952/ 875) 83.3 E10-E03 S23-S06
11 1058 836 (S08W02 L= 93) 219 109 0 (1016/ 820-1092/ 864) 26.6 W00-W04 S09-S06
12 459 785 (S14E38 L= 53) 305 52 0 ( 434/ 771- 493/ 806) 11.3 E40-E35 S14-S12
13 186 743 (S19E70 L= 21) 655 51 0 ( 158/ 720- 218/ 760) 11.3 E79-E63 S20-S17
14 472 733 (S17E37 L= 53) 276 67 2 ( 450/ 708- 496/ 755) 45.0 E39-E35 S18-S15
15 1207 672 (S19W13 L=104) 347 113 1 (1172/ 625-1238/ 712) -45.0 W10-W15 S21-S16
16 1476 528 (S28W35 L=126) 1634 240 2 (1436/ 441-1520/ 652) -63.4 W31-W42 S35-S19
17 801 597 (S25E14 L= 77) 392 113 1 ( 734/ 581- 842/ 623) 7.1 E19-E11 S25-S22
18 1680 495 (S31W58 L=149) 587 93 1 (1637/ 483-1723/ 511) -8.7 W51-W64 S32-S29
|
Download FITS filament maps as tar archive
» All Filament Data of 20230704 ...
|
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.
|
|
|
|