|
|
|
|
| 20240731 - Filament data for 09 UTC |
|
Available data for 20240731: »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
1 660 1592 (N47E24 L=280) 317 70 3 ( 621/1576- 700/1610) 0.0 E27-E19 N45-N48
2 1161 1481 (N32W16 L=319) 1209 305 3 (1025/1428-1300/1523) -27.9 W06-W24 N26-N36
3 1695 1470 (N23W59 L= 2) 470 85 1 (1651/1447-1733/1494) -35.5 W55-W62 N20-N25
4 606 1288 (N26E26 L=278) 261 95 1 ( 564/1275- 657/1298) -8.1 E28-E21 N25-N27
5 716 1172 (N18E18 L=285) 302 100 1 ( 668/1146- 751/1207) 9.5 E21-E15 N16-N20
6 387 1115 (N17E43 L=261) 291 50 2 ( 360/1095- 419/1129) 11.3 E45-E40 N15-N17
7 1496 1004 (S01W29 L=333) 266 135 1 (1450/ 963-1532/1061) -63.4 W26-W31 S04-N02
8 1799 835 (S17W54 L=358) 5821 603 14 (1679/ 611-1935/1015) 42.5 W43-W75 S30-S08
9 1378 841 (S10W20 L=323) 715 164 4 (1330/ 784-1417/ 891) 56.3 W16-W22 S13-S06
10 179 760 (S05E71 L=233) 3501 267 8 ( 139/ 673- 217/ 875) -85.2 E87-E66 S10-N02
11 1533 842 (S12W31 L=334) 388 118 1 (1491/ 799-1562/ 872) -51.3 W27-W32 S14-S09
12 1665 776 (S18W41 L=344) 387 113 1 (1632/ 728-1705/ 806) 33.7 W38-W44 S21-S17
13 1464 714 (S19W25 L=328) 570 195 3 (1386/ 664-1538/ 757) 15.3 W19-W30 S21-S16
14 844 694 (S13E15 L=288) 386 97 0 ( 796/ 673- 891/ 717) -21.8 E17-E12 S14-S10
15 802 533 (S23E21 L=282) 1505 377 3 ( 739/ 443- 923/ 676) 86.4 E24-E13 S29-S13
16 400 534 (S20E53 L=250) 796 149 3 ( 355/ 503- 449/ 573) -23.2 E57-E48 S22-S16
17 611 465 (S26E37 L=266) 384 75 1 ( 592/ 430- 636/ 497) 38.7 E39-E34 S28-S23
18 1594 406 (S45W43 L=346) 1546 186 2 (1544/ 351-1626/ 491) -51.8 W38-W50 S51-S37
19 1045 312 (S43E09 L=294) 570 54 0 (1015/ 285-1079/ 334) 31.0 E11-E06 S45-S41
|
Download FITS filament maps as tar archive
» All Filament Data of 20240731 ...
|
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.
|
|
|
|