|
|
|
|
| 20260312 - Filament data for 09 UTC |
|---|
|
Available data for 20260312: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1330 1589 (N34W03 L= 95) 432 68 1 (1303/1556-1366/1616) 63.4 W01-W04 N31-N37
2 635 1543 (N13E37 L= 55) 777 172 1 ( 571/1492- 704/1575) 54.5 E40-E33 N08-N16
3 1613 1422 (N33W27 L=119) 1105 283 2 (1495/1341-1735/1490) 0.0 W16-W38 N31-N34
4 265 1132 (S18E53 L= 39) 2803 478 4 ( 176/ 941- 377/1297) 64.4 E62-E42 S30-S07
5 141 1187 (S16E70 L= 22) 1258 143 6 ( 105/1126- 175/1242) 49.4 E76-E64 S19-S12
6 671 1084 (S12E22 L= 71) 2002 493 5 ( 434/1034- 856/1141) 22.2 E38-E11 S17-S05
7 1744 1059 (N15W43 L=135) 316 56 1 (1728/1030-1768/1089) -56.3 W41-W45 N13-N16
8 1606 893 (N02W37 L=129) 779 112 2 (1575/ 836-1637/ 943) -80.5 W34-W39 S01-N05
9 1825 838 (N06W57 L=149) 706 100 0 (1806/ 780-1842/ 882) -45.0 W54-W61 N03-N08
10 1416 690 (S14W32 L=124) 532 138 0 (1372/ 642-1469/ 747) -16.7 W27-W37 S15-S12
11 452 641 (S44E31 L= 61) 424 68 1 ( 415/ 616- 476/ 671) 33.7 E34-E28 S45-S41
12 1065 590 (S30W15 L=107) 604 128 0 (1013/ 569-1135/ 624) 20.6 W11-W19 S31-S28
13 598 590 (S44E17 L= 75) 232 25 1 ( 575/ 569- 616/ 609) 33.7 E18-E15 S44-S41
14 794 557 (S40E01 L= 91) 439 80 2 ( 755/ 528- 840/ 583) -11.3 E03-W02 S41-S38
15 1511 489 (S22W48 L=140) 346 67 0 (1494/ 454-1526/ 524) -53.1 W46-W50 S23-S19
16 399 447 (S61E43 L= 49) 671 90 1 ( 364/ 412- 433/ 482) -33.7 E49-E37 S62-S58
17 1564 298 (S29W72 L=164) 567 35 0 (1541/ 280-1589/ 320) 5.7 W66-W76 S30-S28
18 1329 259 (S40W55 L=147) 489 31 0 (1312/ 229-1345/ 289) -18.4 W50-W59 S42-S38
19 1174 232 (S48W47 L=139) 1415 208 2 (1094/ 200-1254/ 278) 19.7 W38-W53 S52-S43
|
|
Data will be available after one hour of observations. |
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.
|
|
|
|
