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| 20140705 - Filament data for 09 UTC |
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Available data for 20140705: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 416 1266 (N17E43 L=220) 823 137 2 ( 373/1214- 447/1336) 90.0 E46-E39 N13-N21
2 925 1200 (N14E07 L=256) 512 228 3 ( 873/1130-1012/1296) -45.0 E10-W00 N09-N20
3 938 1280 (N19E06 L=257) 220 52 0 ( 910/1266- 969/1294) 0.0 E07-E03 N18-N20
4 1097 1196 (N14W04 L=267) 528 221 1 (1029/1137-1151/1288) 60.9 W00-W07 N10-N19
5 212 1192 (N11E62 L=200) 881 180 1 ( 169/1138- 241/1235) -40.6 E68-E58 N07-N13
6 266 1147 (N09E55 L=207) 367 60 0 ( 248/1118- 283/1178) 76.0 E57-E53 N06-N10
7 1244 1111 (N09W14 L=276) 255 68 1 (1215/1079-1268/1150) 68.2 W11-W15 N06-N11
8 991 862 (S07E02 L=261) 253 97 0 ( 961/ 829-1039/ 880) 26.6 E03-W01 S08-S05
9 1072 775 (S12W03 L=266) 291 28 1 (1046/ 746-1095/ 802) -33.7 W01-W04 S13-S10
10 306 705 (S19E53 L=210) 1294 241 4 ( 246/ 627- 353/ 796) -65.6 E57-E48 S24-S13
11 1396 743 (S14W25 L=287) 548 95 1 (1368/ 700-1426/ 790) 59.0 W22-W26 S16-S11
12 1106 716 (S16W06 L=268) 200 79 0 (1078/ 682-1136/ 756) 51.3 W03-W07 S18-S13
13 1000 608 (S23E01 L=261) 505 183 1 ( 980/ 516-1023/ 672) 84.8 E02-W00 S29-S18
14 271 641 (S24E58 L=205) 656 124 1 ( 240/ 618- 302/ 669) -18.4 E61-E54 S25-S21
15 504 596 (S25E37 L=226) 481 168 1 ( 453/ 557- 545/ 655) 33.7 E41-E32 S28-S21
16 706 559 (S27E22 L=241) 421 127 0 ( 688/ 506- 729/ 607) 76.0 E23-E19 S31-S23
17 1267 559 (S26W17 L=280) 633 136 1 (1195/ 535-1310/ 597) 14.0 W12-W20 S28-S23
18 1058 487 (S32W03 L=266) 262 52 0 (1035/ 458-1078/ 516) 53.1 W01-W04 S33-S29
19 402 431 (S39E53 L=210) 553 148 2 ( 386/ 403- 419/ 462) 45.0 E56-E49 S41-S36
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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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