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| 20140106 - Filament data for 08 UTC |
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Available data for 20140106: »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 1337 1629 (N36W23 L=142) 824 255 3 (1217/1599-1439/1654) 6.3 W13-W31 N33-N38
2 1505 1599 (N35W36 L=155) 288 58 0 (1488/1577-1522/1622) 45.0 W33-W37 N32-N36
3 1585 1582 (N34W42 L=161) 318 57 0 (1563/1564-1612/1597) 18.4 W39-W45 N32-N34
4 397 1477 (N25E46 L= 73) 839 322 3 ( 346/1354- 432/1561) -53.7 E53-E41 N16-N31
5 925 1417 (N20E07 L=112) 539 232 1 ( 879/1302- 985/1501) 77.0 E09-E03 N13-N26
6 223 1408 (N21E62 L= 57) 478 74 0 ( 207/1384- 247/1427) -36.9 E64-E58 N19-N22
7 1161 1230 (N09W08 L=127) 192 64 0 (1128/1200-1187/1256) -45.0 W06-W09 N07-N10
8 509 1122 (N02E33 L= 86) 907 235 1 ( 471/ 998- 565/1230) 72.9 E35-E29 S05-N08
9 120 1149 (N06E72 L= 47) 710 192 3 ( 90/1130- 151/1170) 0.0 E78-E66 N04-N06
10 775 1065 (S01E15 L=104) 317 94 3 ( 757/1011- 796/1107) -78.7 E16-E13 S04-N01
11 157 1003 (S04E65 L= 54) 490 96 3 ( 135/ 972- 175/1035) -45.0 E68-E62 S05-S01
12 1868 854 (S11W63 L=182) 2775 492 9 (1796/ 725-1924/ 990) 54.8 W57-W70 S19-S02
13 883 914 (S10E08 L=110) 559 168 1 ( 796/ 878- 963/ 949) 21.8 E13-E03 S12-S08
14 626 859 (S14E25 L= 94) 634 153 4 ( 556/ 820- 690/ 893) -6.3 E29-E20 S15-S11
15 327 771 (S18E49 L= 70) 1155 353 6 ( 244/ 684- 418/ 854) 33.7 E57-E40 S23-S13
16 915 781 (S18E07 L=112) 517 193 4 ( 835/ 745- 986/ 825) 18.4 E11-E02 S20-S15
17 752 747 (S21E17 L=101) 424 188 0 ( 686/ 671- 785/ 800) -58.0 E21-E15 S25-S17
18 967 662 (S26E03 L=115) 586 253 3 ( 843/ 628-1090/ 700) 14.9 E11-W04 S28-S23
19 284 597 (S29E57 L= 62) 944 207 4 ( 256/ 539- 324/ 660) -90.0 E61-E53 S32-S24
20 678 522 (S35E25 L= 93) 337 151 1 ( 641/ 478- 711/ 588) 41.2 E29-E21 S38-S30
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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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