|
|
|
|
| 20240807 - Filament data for 11 UTC |
|
Available data for 20240807: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1164 1669 (N45W25 L=235) 808 163 1 (1105/1629-1244/1699) -45.0 W21-W29 N40-N48
2 636 1584 (N48E23 L=186) 1607 390 3 ( 481/1495- 788/1641) -18.4 E42-E09 N39-N53
3 1605 1537 (N27W54 L=264) 752 122 3 (1542/1504-1634/1573) -29.7 W48-W59 N24-N28
4 1120 1504 (N34W15 L=225) 1354 296 5 ( 988/1477-1273/1529) -11.3 W05-W25 N30-N37
5 1764 1426 (N16W64 L=274) 1408 130 1 (1711/1375-1803/1461) -54.5 W59-W69 N12-N19
6 1778 1267 (N07W58 L=267) 336 33 0 (1754/1247-1795/1285) 0.0 W55-W60 N05-N08
7 511 1016 (N12E33 L=176) 351 107 1 ( 464/ 987- 564/1035) 8.1 E36-E29 N10-N12
8 330 967 (N11E48 L=161) 282 75 0 ( 311/ 942- 358/1004) -63.4 E49-E45 N08-N12
9 287 815 (N01E55 L=155) 1900 487 6 ( 122/ 765- 480/ 905) -11.9 E77-E38 S02-N07
10 791 866 (S00E16 L=193) 331 85 1 ( 757/ 843- 826/ 901) -14.0 E18-E14 S01-N02
11 1293 683 (S19W12 L=221) 2246 487 7 (1207/ 575-1416/ 881) 63.4 W05-W19 S26-S06
12 1136 822 (S07W04 L=213) 341 82 2 (1106/ 790-1160/ 866) 36.9 W01-W05 S09-S05
13 1096 739 (S12W00 L=210) 229 79 0 (1064/ 721-1134/ 761) 0.0 E01-W02 S13-S10
14 1166 700 (S16W04 L=214) 366 180 0 (1090/ 678-1223/ 752) 7.1 W00-W08 S16-S12
15 1556 717 (S21W31 L=240) 463 88 1 (1514/ 690-1597/ 742) 18.4 W27-W34 S22-S20
16 571 645 (S11E35 L=175) 288 74 1 ( 550/ 618- 587/ 678) 45.0 E36-E33 S12-S09
17 477 534 (S18E46 L=163) 1033 262 3 ( 373/ 469- 528/ 633) -63.4 E52-E42 S22-S10
18 713 401 (S30E33 L=176) 531 129 0 ( 676/ 350- 745/ 454) 35.0 E38-E28 S33-S26
|
Download FITS filament maps as tar archive
» All Filament Data of 20240807 ...
|
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.
|
|
|
|