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| 20240822 - Filament data for 10 UTC |
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Available data for 20240822: »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 1606 1624 (N28W63 L= 75) 420 50 0 (1579/1603-1631/1645) -63.4 W60-W64 N25-N29
2 1666 1592 (N24W66 L= 78) 571 54 1 (1640/1569-1686/1614) 15.9 W63-W71 N22-N25
3 618 1440 (N40E21 L=351) 1044 184 1 ( 550/1398- 713/1499) -35.5 E27-E13 N35-N45
4 1282 1331 (N19W22 L= 35) 222 92 0 (1267/1285-1301/1370) 78.7 W21-W24 N16-N21
5 1037 1331 (N25W07 L= 19) 199 123 0 (1000/1298-1090/1346) 0.0 W04-W10 N23-N25
6 170 1286 (N36E73 L=299) 1535 131 3 ( 141/1224- 209/1341) -29.7 E86-E64 N31-N39
7 293 1132 (N25E51 L=321) 533 124 2 ( 256/1084- 316/1186) -45.0 E55-E48 N22-N28
8 225 991 (N17E59 L=313) 615 166 0 ( 181/ 930- 258/1025) -45.0 E64-E55 N13-N19
9 314 934 (N13E50 L=322) 321 99 0 ( 293/ 886- 333/ 979) -71.6 E51-E48 N09-N15
10 404 920 (N11E42 L=330) 347 73 3 ( 370/ 889- 447/ 939) 0.0 E45-E38 N09-N12
11 166 884 (N11E69 L=303) 538 72 2 ( 142/ 852- 188/ 919) 45.0 E72-E64 N08-N13
12 218 804 (N06E63 L=309) 508 58 0 ( 195/ 780- 243/ 827) -31.0 E66-E60 N04-N07
13 425 540 (S13E52 L=320) 2312 503 5 ( 318/ 415- 528/ 666) -72.5 E58-E46 S22-S03
14 610 628 (S09E34 L=338) 468 95 1 ( 578/ 591- 642/ 663) 45.0 E37-E31 S11-S07
15 571 514 (S16E41 L=331) 810 236 2 ( 500/ 440- 663/ 579) -55.0 E44-E36 S22-S11
16 1590 500 (S40W31 L= 43) 571 76 1 (1561/ 475-1617/ 529) 0.0 W28-W34 S42-S37
17 1280 415 (S37W04 L= 16) 279 52 0 (1261/ 390-1304/ 449) 36.9 W02-W06 S39-S35
18 1115 387 (S35E09 L= 3) 249 56 1 (1089/ 370-1141/ 409) 0.0 E10-E06 S36-S33
19 769 314 (S34E36 L=336) 641 181 1 ( 708/ 259- 808/ 381) 26.6 E45-E29 S37-S29
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Download FITS filament maps as tar archive
» All Filament Data of 20240822 ...
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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.
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