|
|
|
|
| 20240722 - Latest Filament data |
|
Available data for 20240722: »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
1 834 1644 (N48E11 L= 50) 436 83 1 ( 804/1605- 856/1673) -51.3 E13-E08 N44-N50
2 1465 1621 (N39W44 L=104) 594 113 0 (1409/1605-1522/1635) -4.8 W38-W50 N37-N39
3 1294 1498 (N32W24 L= 84) 405 79 2 (1262/1460-1325/1532) 51.3 W21-W27 N29-N34
4 1826 1402 (N19W72 L=132) 769 71 2 (1804/1365-1843/1437) 59.0 W68-W76 N16-N21
5 747 948 (N02E18 L= 43) 487 178 0 ( 700/ 880- 809/1010) 36.9 E21-E13 S01-N05
6 513 982 (N05E33 L= 27) 391 115 0 ( 464/ 953- 570/1009) 14.0 E37-E29 N03-N06
7 1511 900 (S07W30 L= 90) 329 63 2 (1496/ 861-1528/ 936) -78.7 W29-W31 S09-S04
8 1446 851 (S09W25 L= 86) 430 150 1 (1409/ 794-1471/ 902) -66.8 W23-W27 S12-S05
9 1562 853 (S10W34 L= 94) 307 63 2 (1539/ 823-1587/ 883) -63.4 W32-W35 S12-S08
10 725 808 (S06E20 L= 40) 284 64 0 ( 708/ 773- 742/ 848) -90.0 E21-E19 S08-S03
11 443 770 (S07E41 L= 19) 512 192 1 ( 357/ 749- 520/ 817) -18.4 E47-E35 S08-S04
12 274 687 (S13E59 L= 1) 616 92 1 ( 256/ 645- 294/ 741) 71.6 E61-E57 S15-S09
13 389 620 (S17E49 L= 11) 900 181 2 ( 340/ 561- 429/ 685) 45.0 E56-E44 S21-S12
14 325 629 (S16E56 L= 4) 409 97 0 ( 311/ 589- 340/ 673) 50.2 E58-E52 S19-S13
15 1571 627 (S25W36 L= 96) 348 95 0 (1538/ 589-1598/ 670) 51.3 W33-W37 S27-S22
16 1689 629 (S27W47 L=107) 548 75 1 (1670/ 584-1710/ 669) 90.0 W45-W48 S30-S24
17 491 448 (S29E47 L= 13) 603 129 3 ( 464/ 399- 516/ 510) 36.9 E53-E41 S33-S24
18 1262 457 (S34W13 L= 73) 427 97 0 (1217/ 439-1316/ 472) -8.1 W09-W16 S35-S32
19 603 367 (S36E41 L= 19) 580 91 2 ( 549/ 351- 653/ 387) -6.3 E46-E36 S37-S34
|
Download FITS filament maps as tar archive
» All Filament Data of 20240722 ...
|
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.
|
|
|
|