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| 20241202 - Filament data for 12 UTC |
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Available data for 20241202: »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 1066 1501 (N28W11 L=116) 962 267 0 ( 966/1403-1159/1589) -60.3 W06-W14 N20-N35
2 723 1440 (N30E13 L= 93) 1314 282 2 ( 662/1316- 814/1546) 45.0 E17-E05 N22-N36
3 1532 1479 (N19W42 L=147) 1104 233 5 (1466/1369-1585/1536) 26.6 W33-W47 N13-N22
4 1348 1483 (N22W29 L=134) 841 222 2 (1243/1437-1451/1524) -36.0 W23-W34 N18-N26
5 433 1351 (N30E35 L= 70) 1349 291 4 ( 314/1306- 586/1390) -19.2 E46-E23 N24-N33
6 1727 1290 (N05W51 L=156) 288 59 0 (1699/1261-1750/1321) -63.4 W49-W52 N02-N06
7 1060 1226 (N12W05 L=110) 735 255 1 ( 948/1159-1129/1301) 22.6 E02-W10 N08-N15
8 1804 1087 (S08W53 L=158) 1515 328 5 (1732/ 991-1866/1194) -72.9 W46-W61 S13-N00
9 1895 1013 (S14W63 L=168) 1341 140 4 (1859/ 953-1920/1084) 63.4 W58-W66 S17-S09
10 673 966 (N03E21 L= 84) 489 171 0 ( 586/ 951- 748/ 984) -11.3 E26-E16 N01-N04
11 1556 821 (S20W30 L=135) 1675 418 4 (1404/ 722-1721/ 960) 17.1 W18-W44 S23-S13
12 727 899 (S02E19 L= 86) 247 46 0 ( 705/ 872- 749/ 926) 33.7 E20-E17 S03-N00
13 900 897 (S05E09 L= 96) 377 160 0 ( 831/ 850- 944/ 922) -45.0 E13-E06 S08-S02
14 432 754 (S06E42 L= 63) 1247 349 3 ( 350/ 618- 520/ 868) -82.4 E46-E37 S14-N01
15 305 714 (S06E54 L= 51) 1696 376 5 ( 257/ 552- 357/ 840) 66.4 E57-E47 S16-N00
16 677 759 (S09E25 L= 80) 298 105 0 ( 640/ 732- 697/ 807) 53.1 E27-E23 S10-S06
17 1662 726 (S27W39 L=144) 471 116 1 (1607/ 708-1729/ 745) -5.2 W33-W44 S28-S25
18 507 443 (S26E48 L= 57) 969 214 0 ( 436/ 377- 593/ 514) 15.9 E59-E38 S28-S22
19 1408 304 (S55W19 L=124) 999 152 0 (1334/ 280-1482/ 337) 0.0 W10-W27 S56-S52
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Download FITS filament maps as tar archive
» All Filament Data of 20241202 ...
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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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