|
|
|
|
| 20240918 - Filament data for 06 UTC |
|
Available data for 20240918: »06 UTC »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
1 271 1305 (N41E53 L=325) 1083 220 1 ( 213/1245- 347/1392) -28.4 E67-E42 N35-N48
2 644 1225 (N28E18 L=359) 301 98 1 ( 593/1211- 696/1238) -23.2 E21-E14 N25-N29
3 1148 1094 (N08W09 L= 26) 326 83 2 (1121/1054-1178/1130) 31.0 W06-W11 N06-N09
4 195 1015 (N24E61 L=317) 2533 320 3 ( 109/ 889- 305/1106) -28.3 E77-E50 N15-N30
5 1306 842 (S10W11 L= 29) 283 125 0 (1283/ 782-1333/ 885) 45.0 W08-W13 S13-S08
6 1126 773 (S09E01 L= 17) 213 106 0 (1088/ 740-1169/ 796) 14.0 E03-W01 S10-S08
7 1097 701 (S13E04 L= 14) 205 50 1 (1070/ 683-1123/ 725) -18.4 E05-E02 S13-S11
8 753 616 (S09E26 L=351) 645 215 0 ( 702/ 531- 800/ 709) 33.7 E32-E20 S13-S04
9 1096 635 (S17E06 L= 12) 325 144 1 (1040/ 609-1138/ 681) 8.1 E09-E02 S18-S14
10 1032 606 (S17E10 L= 7) 209 63 0 (1009/ 591-1061/ 631) -45.0 E11-E08 S18-S14
11 969 503 (S22E18 L= 0) 224 111 0 ( 922/ 482- 999/ 546) 18.4 E20-E14 S22-S19
12 447 475 (S12E54 L=324) 1885 253 9 ( 350/ 431- 534/ 540) -31.6 E63-E47 S16-S07
13 576 455 (S15E45 L=333) 461 120 0 ( 554/ 402- 595/ 516) 33.7 E49-E40 S18-S11
14 1424 446 (S40W10 L= 28) 286 41 2 (1404/ 422-1444/ 467) -76.0 W08-W11 S41-S37
15 627 309 (S26E51 L=327) 912 185 3 ( 585/ 241- 672/ 389) 63.4 E54-E46 S32-S20
16 699 339 (S26E43 L=335) 429 74 2 ( 667/ 309- 732/ 365) 23.2 E46-E39 S27-S24
17 1262 315 (S45E07 L= 11) 372 51 2 (1232/ 294-1295/ 336) -11.3 E09-E03 S46-S42
18 750 163 (S42E59 L=319) 772 64 1 ( 730/ 131- 772/ 192) 32.5 E66-E52 S45-S38
19 1050 130 (S55E40 L=338) 932 104 2 (1010/ 111-1097/ 158) 82.9 E43-E34 S58-S50
|
Download FITS filament maps as tar archive
» All Filament Data of 20240918 ...
|
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.
|
|
|
|