|
|
|
|
| 20240711 - Filament data for 07 UTC |
|
Available data for 20240711: »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 1126 1606 (N42W10 L=219) 577 194 3 (1056/1540-1199/1656) -42.0 W04-W14 N36-N46
2 1220 1525 (N36W16 L=225) 250 54 0 (1200/1497-1237/1554) 63.4 W14-W17 N33-N37
3 1696 1481 (N30W58 L=267) 1108 132 3 (1631/1443-1765/1519) -19.7 W51-W65 N26-N32
4 247 1253 (N18E60 L=149) 1868 236 7 ( 183/1150- 305/1337) 85.2 E67-E54 N11-N23
5 1742 1268 (N16W54 L=263) 562 97 3 (1690/1244-1787/1288) -11.3 W48-W58 N14-N17
6 620 856 (S06E26 L=183) 910 321 0 ( 498/ 769- 715/ 954) -38.2 E34-E20 S11-N00
7 1126 757 (S13W06 L=215) 337 145 1 (1068/ 719-1154/ 809) 56.3 W02-W07 S15-S09
8 462 778 (S11E38 L=170) 279 67 0 ( 437/ 753- 489/ 806) 31.0 E40-E35 S12-S09
9 378 684 (S17E47 L=161) 3013 381 14 ( 253/ 570- 500/ 788) -34.4 E58-E38 S24-S10
10 497 695 (S16E37 L=172) 398 85 2 ( 464/ 659- 521/ 731) -90.0 E39-E34 S18-S13
11 1415 625 (S23W26 L=235) 546 253 3 (1305/ 548-1470/ 691) 42.0 W18-W29 S27-S18
12 697 593 (S23E23 L=185) 920 274 1 ( 633/ 480- 769/ 682) 49.4 E30-E17 S31-S16
13 1266 534 (S28W16 L=225) 1310 295 4 (1209/ 438-1323/ 628) 70.3 W12-W19 S35-S21
14 1106 541 (S27W04 L=213) 261 103 1 (1072/ 508-1146/ 584) 45.0 W02-W07 S29-S24
15 731 419 (S36E24 L=184) 440 88 1 ( 691/ 392- 758/ 448) 33.7 E28-E21 S37-S33
16 616 398 (S38E35 L=173) 433 84 0 ( 587/ 374- 652/ 431) -26.6 E37-E31 S39-S34
17 1109 364 (S41W05 L=214) 420 36 2 (1085/ 339-1136/ 386) -45.0 W03-W07 S43-S39
18 900 192 (S58E18 L=191) 491 56 0 ( 881/ 167- 917/ 220) 49.4 E22-E15 S61-S54
|
Download FITS filament maps as tar archive
» All Filament Data of 20240711 ...
|
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.
|
|
|
|