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| 20230111 - Filament data for 11 UTC |
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Available data for 20230111: »07 UTC »08 UTC »09 UTC »10 UTC »11 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 1418 1653 (N39W28 L=255) 1965 315 3 (1289/1577-1559/1710) -18.4 W17-W39 N34-N43
2 337 1498 (N24E55 L=172) 835 109 6 ( 316/1449- 360/1559) -53.1 E59-E51 N20-N28
3 913 1534 (N27E10 L=217) 240 85 1 ( 877/1511- 951/1557) -18.4 E12-E06 N25-N28
4 1688 1417 (N24W47 L=274) 406 86 1 (1667/1383-1710/1464) -80.5 W44-W48 N21-N27
5 1530 1170 (N07W31 L=258) 439 118 0 (1495/1136-1550/1232) -90.0 W28-W32 N05-N10
6 412 1093 (S01E40 L=187) 227 74 1 ( 394/1053- 427/1127) -71.6 E41-E38 S03-N00
7 254 958 (S09E54 L=173) 312 39 1 ( 232/ 941- 278/ 977) -14.0 E56-E51 S10-S08
8 488 904 (S13E34 L=193) 498 147 0 ( 454/ 842- 531/ 962) 49.4 E37-E30 S16-S09
9 278 844 (S16E53 L=174) 546 97 2 ( 242/ 815- 328/ 875) -20.6 E56-E47 S17-S14
10 1074 809 (S17W04 L=231) 216 47 1 (1053/ 789-1094/ 841) -90.0 W02-W05 S18-S14
11 927 784 (S19E05 L=222) 229 126 1 ( 888/ 752- 991/ 835) 39.8 E07-E01 S20-S15
12 1723 761 (S16W50 L=278) 482 92 4 (1695/ 718-1751/ 802) -59.0 W47-W53 S18-S13
13 462 628 (S30E40 L=187) 966 142 2 ( 433/ 561- 500/ 706) 84.3 E41-E36 S34-S24
14 211 609 (S30E72 L=155) 1265 67 1 ( 186/ 570- 238/ 642) 12.5 E84-E64 S32-S28
15 1372 594 (S29W26 L=253) 588 110 3 (1328/ 559-1401/ 639) 59.0 W23-W28 S31-S25
16 1115 587 (S31W08 L=235) 499 186 0 (1024/ 572-1202/ 601) 4.4 W01-W14 S31-S29
17 664 534 (S36E25 L=202) 257 101 1 ( 619/ 521- 719/ 552) 0.0 E28-E20 S36-S34
18 864 493 (S38E10 L=217) 254 73 0 ( 827/ 468- 893/ 523) 31.0 E12-E07 S40-S36
19 573 276 (S57E50 L=177) 468 39 1 ( 550/ 255- 602/ 299) 13.0 E56-E43 S58-S54
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Download FITS filament maps as tar archive
» All Filament Data of 20230111 ...
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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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