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| 20240908 - Latest Filament data |
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Available data for 20240908: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 935 1655 (N47W14 L=161) 363 108 0 ( 904/1614- 977/1694) 18.4 W10-W19 N45-N49
2 1035 1398 (N28W11 L=157) 450 123 1 ( 974/1359-1082/1427) 6.3 W05-W14 N26-N29
3 1158 1248 (N16W13 L=160) 214 122 0 (1099/1232-1207/1271) -18.4 W10-W16 N15-N18
4 1894 1172 (S09W67 L=213) 2800 150 4 (1843/1110-1938/1259) 14.0 W58-W75 S13-S04
5 717 1203 (N24E14 L=132) 826 206 2 ( 630/1145- 803/1258) 0.0 E21-E08 N22-N26
6 423 1106 (N25E37 L=109) 430 135 1 ( 369/1063- 477/1143) 11.3 E42-E32 N22-N26
7 1513 846 (S15W25 L=171) 2382 619 10 (1318/ 717-1649/1082) 22.5 W09-W39 S19-S05
8 1835 948 (S20W53 L=200) 653 152 0 (1801/ 890-1857/1027) 36.9 W49-W57 S22-S15
9 275 896 (N15E54 L= 93) 300 53 0 ( 262/ 867- 288/ 930) 76.0 E55-E52 N12-N16
10 1525 911 (S12W27 L=173) 310 51 0 (1497/ 886-1550/ 929) -33.7 W24-W28 S13-S10
11 540 609 (S06E40 L=107) 854 245 0 ( 439/ 551- 635/ 688) -50.7 E45-E34 S11-N00
12 1544 603 (S32W23 L=170) 517 121 0 (1484/ 571-1591/ 635) 0.0 W18-W27 S32-S30
13 1195 540 (S25E02 L=145) 377 74 1 (1152/ 508-1221/ 566) -36.9 E04-W00 S27-S23
14 1103 485 (S27E09 L=138) 374 148 1 (1073/ 431-1152/ 538) 32.0 E12-E04 S29-S23
15 828 435 (S23E28 L=119) 457 133 0 ( 791/ 392- 863/ 499) 32.0 E31-E23 S25-S19
16 1170 392 (S35E08 L=139) 918 195 3 (1095/ 323-1231/ 473) 31.6 E15-E02 S38-S30
17 663 373 (S24E42 L=104) 1008 221 3 ( 614/ 303- 732/ 457) -90.0 E46-E38 S29-S17
18 1426 368 (S46W10 L=157) 551 90 1 (1381/ 342-1461/ 399) 0.0 W06-W13 S47-S43
19 1061 137 (S56E35 L=111) 519 52 0 (1042/ 114-1078/ 169) 32.5 E40-E29 S59-S52
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Download FITS filament maps as tar archive
» All Filament Data of 20240908 ...
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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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