|
|
|
|
| 20230613 - Filament data for 08 UTC |
|
Available data for 20230613: »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 1282 1837 (N67W14 L= 24) 664 76 1 (1247/1809-1316/1855) 0.0 W08-W19 N63-N69
2 1434 1446 (N33W24 L= 34) 1255 322 2 (1381/1326-1542/1541) -49.8 W19-W32 N25-N39
3 508 1437 (N20E42 L=328) 400 79 0 ( 471/1414- 549/1460) -15.9 E45-E38 N18-N20
4 865 1412 (N23E16 L=354) 281 62 1 ( 848/1388- 887/1444) 90.0 E17-E13 N21-N24
5 1730 1346 (N30W51 L= 61) 406 47 2 (1708/1315-1756/1377) 63.4 W48-W54 N27-N31
6 1333 1285 (N21W17 L= 27) 321 129 1 (1297/1246-1385/1334) -45.0 W13-W20 N18-N23
7 675 1272 (N11E25 L=345) 240 51 1 ( 645/1254- 704/1293) 0.0 E27-E23 N10-N12
8 1363 1197 (N15W19 L= 29) 233 75 1 (1329/1176-1393/1217) -11.3 W16-W21 N14-N16
9 1501 1035 (N07W30 L= 40) 292 68 1 (1485/1007-1515/1071) -76.0 W29-W31 N05-N09
10 872 807 (S14E07 L= 3) 442 173 0 ( 817/ 745- 922/ 882) 60.9 E09-E04 S18-S09
11 1490 825 (S06W32 L= 42) 293 83 1 (1468/ 783-1521/ 852) 59.0 W31-W34 S08-S03
12 462 732 (S25E36 L=334) 944 171 1 ( 437/ 659- 486/ 822) 74.7 E38-E33 S29-S18
13 1494 711 (S13W35 L= 45) 251 91 0 (1456/ 683-1535/ 736) 45.0 W32-W37 S14-S10
14 1187 690 (S18W15 L= 25) 292 79 0 (1161/ 657-1223/ 717) 53.1 W13-W16 S19-S15
15 1426 561 (S23W34 L= 44) 283 120 0 (1411/ 528-1459/ 603) -78.7 W32-W37 S25-S20
16 1080 550 (S28W10 L= 20) 854 194 1 ( 983/ 521-1156/ 593) 28.6 W03-W14 S31-S24
17 540 536 (S37E31 L=339) 968 148 2 ( 512/ 472- 584/ 577) -90.0 E33-E26 S42-S34
18 1536 486 (S27W47 L= 57) 3016 559 2 (1314/ 433-1779/ 568) 18.4 W30-W72 S33-S18
19 1277 536 (S27W24 L= 34) 374 115 0 (1231/ 500-1323/ 558) 45.0 W22-W27 S29-S24
|
Download FITS filament maps as tar archive
» All Filament Data of 20230613 ...
|
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.
|
|
|
|