|
|
|
|
| 20240114 - Filament data for 09 UTC |
|
Available data for 20240114: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 449 1669 (N36E54 L=357) 2227 201 3 ( 392/1573- 499/1721) -24.8 E70-E44 N28-N40
2 916 1682 (N38E13 L= 38) 411 103 1 ( 875/1662- 967/1714) -14.0 E16-E08 N36-N40
3 626 1392 (N16E28 L= 23) 664 162 0 ( 591/1325- 671/1464) 71.6 E29-E25 N12-N21
4 1650 1427 (N25W43 L= 94) 603 89 0 (1602/1390-1690/1457) -23.2 W38-W46 N22-N26
5 1355 1399 (N21W19 L= 70) 278 87 0 (1311/1371-1394/1431) -31.0 W16-W21 N18-N22
6 788 1357 (N15E16 L= 35) 406 139 0 ( 725/1320- 842/1379) -14.0 E20-E12 N12-N16
7 736 1268 (N09E19 L= 32) 227 96 0 ( 699/1229- 759/1292) -36.9 E21-E17 N06-N10
8 187 1210 (N05E63 L=348) 957 128 4 ( 168/1154- 209/1265) 90.0 E65-E60 N01-N08
9 595 1179 (N03E27 L= 24) 318 93 0 ( 573/1138- 624/1227) -63.4 E28-E25 N00-N06
10 195 1094 (S02E60 L=351) 1096 176 1 ( 154/1034- 224/1186) 48.8 E65-E57 S05-N03
11 309 847 (S17E50 L= 1) 601 122 2 ( 266/ 796- 345/ 893) 45.0 E54-E46 S20-S14
12 553 864 (S16E30 L= 21) 599 218 0 ( 452/ 838- 650/ 885) 7.6 E37-E22 S17-S14
13 1386 809 (S15W24 L= 75) 264 69 0 (1370/ 776-1406/ 844) -63.4 W22-W25 S16-S12
14 1497 744 (S18W33 L= 84) 341 68 0 (1463/ 725-1529/ 767) 36.9 W30-W34 S19-S16
15 1533 676 (S22W37 L= 88) 994 282 2 (1465/ 576-1617/ 756) 63.4 W32-W42 S28-S16
16 1282 706 (S22W19 L= 70) 360 142 0 (1222/ 683-1352/ 741) -12.5 W14-W23 S23-S20
17 1439 571 (S29W33 L= 84) 314 76 0 (1418/ 550-1469/ 605) -45.0 W30-W35 S30-S27
18 1587 480 (S34W50 L=101) 837 99 3 (1551/ 453-1627/ 524) -12.5 W45-W54 S35-S30
19 1221 421 (S42W20 L= 71) 311 54 0 (1197/ 402-1255/ 447) 0.0 W17-W23 S43-S39
|
Download FITS filament maps as tar archive
» All Filament Data of 20240114 ...
|
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.
|
|
|
|