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| 20131118 - Filament data for 08 UTC |
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Available data for 20131118: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1239 1414 (N20W22 L= 66) 348 153 1 (1179/1358-1297/1453) -69.4 W18-W24 N15-N23
2 1114 1399 (N22W14 L= 58) 288 85 1 (1098/1357-1137/1442) 78.7 W12-W14 N19-N24
3 545 1410 (N36E24 L= 20) 287 81 0 ( 508/1395- 586/1427) 0.0 E27-E20 N34-N36
4 903 1394 (N26W01 L= 45) 1170 263 2 ( 795/1344-1018/1419) -26.6 E06-W06 N20-N29
5 1061 1264 (N15W07 L= 52) 225 44 0 (1029/1248-1092/1278) -26.6 W05-W09 N14-N16
6 275 1211 (N29E50 L=355) 374 49 1 ( 251/1184- 302/1234) 33.7 E52-E46 N26-N29
7 758 1179 (N17E12 L= 32) 551 144 1 ( 698/1142- 828/1215) -40.6 E15-E08 N13-N19
8 361 1135 (N22E41 L= 3) 881 28 1 ( 288/1073- 445/1204) -37.6 E48-E35 N17-N27
9 1643 1107 (S06W40 L= 84) 480 140 0 (1611/1067-1681/1157) -80.5 W37-W42 S08-S02
10 1821 1024 (S15W54 L= 99) 2314 274 7 (1782/ 912-1860/1149) 85.9 W49-W59 S21-S07
11 1020 1109 (N07W01 L= 46) 182 81 1 ( 973/1089-1052/1123) -14.0 E01-W03 N05-N08
12 1728 1014 (S14W45 L= 90) 554 124 4 (1670/ 988-1780/1044) -18.4 W40-W49 S16-S11
13 195 938 (N13E61 L=344) 397 59 2 ( 179/ 910- 214/ 971) 63.4 E63-E58 N11-N15
14 1213 817 (S13W07 L= 51) 294 71 0 (1192/ 789-1242/ 846) 33.7 W05-W08 S14-S11
15 1347 769 (S19W14 L= 58) 245 70 0 (1328/ 746-1377/ 797) 71.6 W12-W15 S20-S17
16 550 747 (S04E35 L= 10) 391 103 1 ( 511/ 716- 580/ 773) -36.9 E37-E32 S05-S02
17 444 635 (S08E46 L=359) 430 76 2 ( 426/ 599- 466/ 680) 68.2 E47-E43 S10-S05
18 645 409 (S26E42 L= 3) 1909 370 1 ( 603/ 261- 671/ 570) 51.0 E54-E35 S36-S15
19 275 531 (S12E69 L=335) 587 52 3 ( 248/ 509- 297/ 561) 5.7 E74-E64 S13-S10
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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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