|
|
|
|
| 20240312 - Filament data for 11 UTC |
|
Available data for 20240312: »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1022 1718 (N35E22 L=344) 1463 255 1 ( 951/1614-1093/1805) -26.6 E32-E12 N29-N40
2 637 1646 (N20E43 L=323) 1070 227 1 ( 561/1584- 737/1676) 41.6 E46-E36 N14-N23
3 463 1537 (N09E51 L=316) 808 158 1 ( 438/1468- 491/1607) -52.1 E54-E46 N05-N14
4 1415 1485 (N31W11 L= 18) 1264 246 2 (1328/1399-1490/1540) -15.9 W04-W18 N26-N33
5 330 1467 (N03E59 L=307) 540 125 1 ( 314/1407- 346/1522) -40.6 E63-E55 N00-N06
6 1059 1358 (N12E07 L=360) 584 165 0 (1019/1292-1123/1412) 71.6 E07-E04 N07-N16
7 1277 1254 (N12W08 L= 14) 787 256 3 (1202/1155-1353/1357) -28.3 W01-W14 N08-N16
8 216 1240 (S12E63 L=304) 521 84 0 ( 177/1223- 262/1258) 16.7 E67-E57 S13-S10
9 277 1038 (S23E52 L=315) 581 196 0 ( 210/ 983- 349/1096) 34.7 E58-E45 S27-S18
10 344 839 (S34E43 L=323) 779 180 0 ( 275/ 787- 407/ 905) 35.5 E51-E37 S38-S28
11 1521 670 (S12W40 L= 47) 666 194 0 (1447/ 609-1603/ 712) 59.0 W37-W44 S17-S07
12 1062 639 (S28W13 L= 20) 934 199 2 ( 978/ 594-1139/ 707) 61.4 W09-W16 S32-S21
13 1681 592 (S11W57 L= 63) 468 73 2 (1659/ 559-1716/ 617) 68.2 W54-W59 S13-S08
14 345 568 (S53E48 L=319) 344 23 0 ( 324/ 552- 364/ 589) 20.6 E51-E43 S54-S50
15 1717 541 (S12W64 L= 70) 415 67 1 (1685/ 519-1742/ 566) 45.0 W61-W65 S14-S10
16 1615 468 (S20W59 L= 66) 2012 203 4 (1556/ 429-1707/ 522) 20.6 W52-W69 S22-S15
17 1357 449 (S29W41 L= 47) 720 132 0 (1286/ 431-1426/ 468) 29.1 W36-W45 S32-S26
18 1612 399 (S23W66 L= 72) 851 80 2 (1569/ 361-1646/ 421) 0.0 W59-W74 S24-S21
19 1159 353 (S42W35 L= 41) 330 50 1 (1134/ 322-1175/ 387) -38.7 W32-W37 S43-S39
|
Download FITS filament maps as tar archive
» All Filament Data of 20240312 ...
|
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.
|
|
|
|