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| 20230310 - Filament data for 10 UTC |
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Available data for 20230310: »07 UTC »08 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 740 1760 (N30E43 L=140) 1859 349 5 ( 661/1660- 831/1819) -82.4 E49-E33 N21-N36
2 1160 1719 (N39E13 L=171) 632 141 2 (1110/1665-1198/1770) -26.6 E18-E08 N35-N42
3 511 1657 (N18E54 L=130) 373 54 2 ( 487/1626- 535/1679) -56.3 E56-E51 N16-N20
4 353 1510 (N06E59 L=124) 730 125 0 ( 304/1472- 402/1546) 45.0 E63-E55 N03-N09
5 1719 1402 (N36W38 L=222) 726 187 0 (1689/1303-1748/1476) -59.0 W35-W41 N29-N40
6 238 1110 (S19E57 L=127) 397 70 2 ( 218/1076- 257/1140) -76.0 E58-E54 S21-S17
7 1833 1082 (N20W53 L=236) 576 117 0 (1815/1028-1859/1133) 81.9 W50-W55 N16-N23
8 452 963 (S24E35 L=149) 446 109 1 ( 425/ 931- 504/1006) -26.6 E37-E30 S25-S21
9 663 933 (S21E19 L=164) 450 169 2 ( 603/ 858- 706/ 985) -32.0 E23-E15 S24-S18
10 1682 922 (N05W43 L=226) 351 63 1 (1653/ 893-1703/ 950) -45.0 W40-W44 N03-N06
11 194 872 (S34E62 L=122) 673 110 1 ( 177/ 817- 215/ 927) 54.5 E65-E58 S37-S30
12 314 833 (S35E46 L=137) 410 130 0 ( 295/ 775- 343/ 889) -56.3 E48-E43 S37-S30
13 1431 825 (S07W29 L=212) 335 73 1 (1410/ 784-1450/ 858) 90.0 W26-W30 S09-S05
14 1604 651 (S11W47 L=230) 1140 258 1 (1496/ 587-1701/ 717) 55.3 W42-W52 S17-S04
15 1307 512 (S28W34 L=217) 522 152 0 (1236/ 490-1366/ 547) 35.5 W28-W36 S29-S23
16 1513 385 (S28W57 L=241) 1834 281 4 (1379/ 351-1633/ 417) 15.1 W46-W73 S32-S23
17 602 343 (S64E14 L=169) 1695 239 2 ( 505/ 303- 703/ 397) 0.0 E29-W00 S66-S60
18 1196 336 (S42W38 L=222) 1334 157 5 (1119/ 305-1275/ 373) 22.6 W30-W44 S44-S38
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Download FITS filament maps as tar archive
» All Filament Data of 20230310 ...
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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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