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| 20140108 - Filament data for 10 UTC |
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Available data for 20140108: »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 1346 1521 (N28W21 L=112) 359 45 0 (1312/1495-1378/1548) -45.0 W18-W23 N26-N30
2 333 1447 (N22E51 L= 40) 444 89 1 ( 313/1412- 358/1480) -53.1 E53-E48 N20-N24
3 1389 1448 (N23W23 L=115) 323 58 1 (1354/1426-1416/1468) 21.8 W20-W25 N22-N24
4 521 1439 (N21E35 L= 56) 323 96 0 ( 472/1425- 562/1451) -8.1 E38-E31 N20-N22
5 283 1193 (N06E52 L= 40) 511 142 1 ( 264/1140- 311/1273) -63.4 E53-E48 N03-N11
6 148 1162 (N05E67 L= 24) 1408 225 3 ( 116/1094- 183/1222) 45.0 E72-E62 N01-N08
7 960 1125 (N02E04 L= 87) 514 141 2 ( 923/1082- 986/1196) 71.6 E06-E02 N00-N06
8 985 1033 (S03E02 L= 89) 174 114 0 ( 961/ 980-1035/1062) 59.0 E03-W00 S06-S01
9 1208 1016 (S04W11 L=102) 281 74 3 (1155/ 994-1249/1035) 0.0 W07-W13 S05-S02
10 1292 877 (S12W17 L=108) 192 92 0 (1246/ 866-1342/ 893) 18.4 W13-W20 S12-S10
11 1770 860 (S11W52 L=144) 414 93 2 (1740/ 822-1794/ 886) -31.0 W49-W54 S12-S09
12 1364 773 (S18W22 L=114) 694 193 1 (1272/ 734-1426/ 852) 33.7 W16-W25 S20-S12
13 918 737 (S21E06 L= 85) 718 178 1 ( 887/ 640- 946/ 821) 84.8 E08-E04 S27-S16
14 314 769 (S19E50 L= 41) 732 211 5 ( 252/ 719- 365/ 810) 18.4 E56-E44 S22-S16
15 619 743 (S21E26 L= 65) 361 75 0 ( 588/ 712- 661/ 775) 38.7 E28-E23 S23-S19
16 1295 657 (S26W19 L=110) 1167 441 3 (1169/ 612-1496/ 743) 9.9 W10-W33 S28-S20
17 256 610 (S29E60 L= 32) 1487 387 3 ( 226/ 511- 286/ 685) 39.8 E66-E54 S35-S24
18 557 539 (S35E34 L= 57) 322 118 2 ( 542/ 488- 576/ 583) 60.3 E36-E31 S38-S31
19 1046 526 (S35W03 L= 94) 334 90 0 (1001/ 492-1084/ 569) 45.0 W00-W05 S37-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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