|
|
|
|
| 20230211 - Filament data for 11 UTC |
|
Available data for 20230211: »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
1 747 1646 (N27E31 L=147) 747 142 1 ( 718/1592- 796/1694) 90.0 E33-E28 N23-N31
2 365 1558 (N16E59 L=120) 4812 300 10 ( 288/1432- 433/1650) -38.3 E77-E49 N07-N22
3 821 1439 (N14E20 L=159) 204 51 0 ( 795/1426- 853/1455) 0.0 E21-E17 N13-N15
4 1711 1331 (N26W41 L=220) 939 149 3 (1665/1266-1776/1375) -21.8 W37-W47 N23-N28
5 1894 1212 (N24W63 L=242) 1013 117 3 (1856/1154-1927/1255) -20.0 W57-W68 N20-N26
6 307 1122 (S11E50 L=129) 421 68 0 ( 280/1096- 340/1153) 36.9 E52-E46 S12-S09
7 269 1017 (S18E52 L=127) 1601 247 4 ( 215/ 912- 325/1099) -45.0 E58-E46 S23-S12
8 512 981 (S17E31 L=147) 213 77 0 ( 480/ 951- 543/1011) 45.0 E33-E29 S19-S15
9 1343 890 (S08W21 L=200) 210 66 0 (1309/ 865-1373/ 913) 45.0 W19-W22 S10-S06
10 602 750 (S30E23 L=156) 239 33 1 ( 580/ 730- 620/ 778) 56.3 E24-E21 S31-S27
11 729 735 (S29E14 L=165) 676 193 0 ( 644/ 709- 821/ 773) 0.0 E19-E07 S29-S27
12 520 740 (S32E29 L=149) 246 64 0 ( 486/ 726- 559/ 759) 0.0 E32-E26 S32-S30
13 1830 608 (S12W73 L=251) 860 89 3 (1810/ 553-1850/ 643) -50.2 W68-W77 S15-S09
14 283 600 (S44E59 L=120) 788 80 0 ( 237/ 571- 324/ 631) 12.5 E69-E51 S46-S41
15 1507 568 (S23W42 L=221) 609 260 0 (1393/ 523-1608/ 626) 39.8 W35-W48 S27-S17
16 460 433 (S55E42 L=137) 1372 187 3 ( 377/ 385- 559/ 476) 14.0 E63-E27 S59-S49
17 1618 379 (S31W67 L=245) 3882 281 6 (1484/ 336-1739/ 438) 27.6 W54-W81 S36-S24
18 1308 294 (S45W46 L=224) 338 42 0 (1282/ 276-1337/ 310) 56.3 W43-W47 S46-S43
|
Download FITS filament maps as tar archive
» All Filament Data of 20230211 ...
|
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.
|
|
|
|