|
|
|
|
| 20241006 - Filament data for 08 UTC |
|
Available data for 20241006: »06 UTC »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 1603 1520 (N16W53 L=192) 386 68 1 (1567/1498-1637/1538) -31.0 W50-W56 N14-N17
2 1739 1438 (N07W60 L=199) 568 92 1 (1694/1409-1770/1475) -5.2 W54-W65 N05-N08
3 1583 1301 (N05W41 L=180) 232 64 0 (1551/1287-1614/1313) -36.9 W38-W43 N03-N06
4 1852 1117 (S14W58 L=197) 5366 535 18 (1783/ 875-1922/1280) 51.0 W49-W71 S28-S05
5 1025 1257 (N19W06 L=145) 481 140 2 ( 948/1237-1093/1275) -32.0 W02-W10 N16-N21
6 858 1164 (N18E06 L=133) 360 170 0 ( 788/1113- 915/1208) -49.4 E09-E03 N14-N21
7 1694 1165 (S06W44 L=183) 287 58 0 (1680/1136-1709/1193) 26.6 W42-W46 S06-S04
8 286 975 (N21E50 L= 89) 2088 378 2 ( 183/ 838- 370/1145) -55.7 E61-E45 N11-N33
9 1768 1014 (S16W46 L=185) 754 96 1 (1736/ 963-1795/1066) 80.5 W43-W48 S19-S13
10 500 983 (N17E32 L=107) 355 110 1 ( 455/ 948- 558/1016) -50.2 E35-E28 N13-N19
11 710 936 (N10E20 L=119) 188 81 1 ( 678/ 910- 723/ 978) 45.0 E22-E18 N08-N11
12 1239 806 (S11W06 L=145) 879 337 4 (1190/ 647-1261/ 959) 58.0 W00-W10 S19-S03
13 1638 900 (S18W33 L=172) 659 219 1 (1543/ 872-1730/ 936) -10.6 W25-W41 S20-S15
14 1373 560 (S30W08 L=147) 3299 596 10 (1219/ 378-1527/ 796) 29.5 E08-W22 S38-S19
15 1125 679 (S15E04 L=135) 230 108 0 (1078/ 646-1164/ 692) -45.0 E06-E01 S18-S13
16 569 612 (S05E38 L=101) 911 230 2 ( 519/ 499- 598/ 681) 65.6 E43-E34 S11-N00
17 382 618 (S01E52 L= 87) 1592 218 5 ( 275/ 573- 470/ 673) -29.7 E61-E46 S05-N03
18 764 438 (S20E33 L=106) 1121 322 2 ( 742/ 302- 796/ 589) 48.4 E41-E25 S29-S11
19 958 507 (S21E19 L=120) 401 124 1 ( 936/ 452- 977/ 579) 58.0 E21-E15 S24-S16
|
Download FITS filament maps as tar archive
» All Filament Data of 20241006 ...
|
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.
|
|
|
|