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| 20140101 - Filament data for 10 UTC |
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Available data for 20140101: »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 1480 1662 (N38W37 L=221) 413 63 2 (1454/1636-1508/1683) 0.0 W35-W40 N36-N39
2 409 1584 (N35E47 L=137) 480 79 1 ( 369/1566- 444/1604) 18.4 E50-E43 N33-N36
3 673 1577 (N33E24 L=159) 569 159 0 ( 600/1563- 758/1590) -4.4 E30-E17 N31-N34
4 1590 1370 (N18W38 L=222) 931 298 1 (1470/1314-1723/1439) -18.4 W30-W48 N14-N22
5 378 1301 (N15E43 L=141) 587 149 3 ( 334/1256- 420/1341) -36.9 E47-E39 N12-N18
6 955 1175 (N06E04 L=180) 712 197 1 ( 856/1103-1025/1229) -37.9 E09-W00 N01-N09
7 946 944 (S08E05 L=179) 691 206 1 ( 891/ 845-1025/1022) 51.3 E08-W00 S13-S03
8 1557 932 (S09W34 L=217) 388 81 2 (1518/ 897-1587/ 965) 45.0 W31-W35 S10-S06
9 1181 887 (S11W09 L=193) 187 85 0 (1157/ 858-1223/ 906) 26.6 W07-W11 S13-S10
10 1262 825 (S15W14 L=198) 507 249 0 (1186/ 784-1367/ 867) 22.6 W09-W21 S17-S12
11 336 790 (S15E48 L=136) 625 113 1 ( 302/ 753- 386/ 831) 14.0 E51-E42 S17-S12
12 1635 792 (S17W41 L=224) 269 66 0 (1618/ 765-1651/ 817) 71.6 W39-W42 S18-S15
13 599 777 (S17E28 L=156) 285 60 0 ( 583/ 750- 622/ 810) 76.0 E29-E26 S18-S14
14 1814 769 (S18W57 L=241) 647 79 0 (1777/ 733-1846/ 799) 38.7 W53-W60 S20-S16
15 158 737 (S17E68 L=116) 939 205 2 ( 130/ 706- 189/ 778) 29.7 E73-E63 S18-S14
16 1813 656 (S25W60 L=243) 538 150 2 (1774/ 639-1853/ 677) 0.0 W55-W64 S26-S23
17 229 615 (S25E63 L=121) 576 276 0 ( 202/ 566- 266/ 662) 26.6 E67-E57 S27-S22
18 338 513 (S32E55 L=128) 1407 308 3 ( 309/ 417- 365/ 650) 60.6 E59-E48 S39-S23
19 1210 520 (S35W13 L=196) 1011 191 0 (1134/ 444-1287/ 596) 47.7 W07-W17 S40-S29
20 620 439 (S39E33 L=150) 1565 397 4 ( 558/ 367- 673/ 532) 38.2 E41-E27 S44-S32
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Data will be available after one hour of observations. |
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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