|
|
|
|
| 20250801 - Filament data for 10 UTC |
|
Available data for 20250801: »06 UTC »07 UTC »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 1507 1758 (N45W66 L=218) 631 60 1 (1471/1738-1535/1778) 3.6 W58-W74 N44-N46
2 1293 1733 (N48W38 L=190) 325 40 1 (1275/1704-1313/1756) 38.7 W35-W40 N46-N50
3 660 1699 (N56E27 L=125) 479 68 0 ( 634/1667- 690/1725) 68.2 E29-E23 N53-N58
4 424 1672 (N55E62 L= 90) 1049 96 1 ( 371/1648- 476/1691) -1.7 E84-E51 N53-N56
5 774 1384 (N31E13 L=139) 225 68 0 ( 749/1356- 793/1417) 45.0 E14-E11 N28-N32
6 606 1357 (N30E26 L=126) 1083 212 4 ( 506/1326- 711/1377) -3.4 E34-E17 N28-N32
7 518 1113 (N16E32 L=120) 565 201 0 ( 479/1035- 553/1191) 66.0 E35-E29 N11-N20
8 954 986 (N04E05 L=147) 978 402 0 ( 869/ 814-1001/1129) -75.3 E08-E02 S06-N13
9 1658 951 (S07W41 L=193) 763 146 4 (1612/ 901-1733/1004) -41.2 W37-W47 S10-S03
10 882 768 (S08E11 L=141) 272 114 0 ( 831/ 733- 937/ 785) -26.6 E14-E08 S10-S06
11 1832 729 (S24W60 L=212) 906 92 2 (1813/ 686-1852/ 778) -60.3 W57-W63 S27-S20
12 1763 662 (S28W53 L=205) 672 96 2 (1736/ 621-1787/ 714) 71.6 W50-W55 S30-S24
13 1304 623 (S22W14 L=166) 929 175 4 (1248/ 558-1359/ 694) 48.8 W09-W17 S26-S18
14 739 625 (S16E23 L=129) 312 52 1 ( 717/ 601- 762/ 658) 45.0 E24-E21 S17-S13
15 1456 485 (S35W25 L=177) 3021 497 4 (1299/ 403-1607/ 626) 14.6 W12-W36 S40-S26
16 839 471 (S27E19 L=132) 436 109 1 ( 806/ 450- 891/ 501) -31.0 E21-E15 S29-S24
17 636 400 (S31E38 L=114) 661 101 1 ( 596/ 370- 675/ 430) 18.4 E41-E32 S33-S28
18 1466 286 (S54W34 L=186) 1108 117 2 (1400/ 266-1521/ 310) -14.7 W24-W43 S57-S50
|
Download FITS filament maps as tar archive
» All Filament Data of 20250801 ...
|
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.
|
|
|
|