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| 20140417 - Filament data for 06 UTC |
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Available data for 20140417: »06 UTC »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
1 472 1670 (N18E59 L=170) 1218 131 3 ( 411/1629- 524/1706) 60.3 E63-E55 N14-N21
2 628 1578 (N16E41 L=188) 291 85 0 ( 597/1547- 651/1604) -18.4 E44-E38 N14-N17
3 564 1441 (N06E40 L=190) 464 78 0 ( 523/1423- 606/1457) 31.0 E42-E36 N04-N08
4 449 1233 (S08E41 L=189) 942 274 0 ( 415/1104- 476/1355) -60.3 E46-E37 S15-S01
5 1175 1313 (N15W00 L=230) 244 91 1 (1139/1270-1196/1355) 90.0 W00-W01 N11-N17
6 1486 1280 (N22W20 L=249) 361 53 1 (1471/1251-1511/1317) -63.4 W18-W22 N20-N24
7 328 1087 (S19E46 L=183) 728 220 0 ( 256/1057- 407/1124) 22.6 E52-E40 S21-S15
8 738 1046 (S12E17 L=212) 242 93 0 ( 688/1026- 780/1058) 31.0 E19-E13 S14-S10
9 813 755 (S26E05 L=224) 304 97 0 ( 797/ 705- 840/ 803) -59.0 E06-E01 S28-S23
10 247 772 (S41E51 L=179) 605 131 1 ( 210/ 756- 292/ 801) 6.3 E54-E45 S41-S38
11 921 601 (S32W07 L=236) 1156 293 1 ( 779/ 531-1060/ 707) -2.5 E05-W18 S34-S29
12 1133 595 (S26W20 L=249) 343 87 1 (1103/ 569-1176/ 638) -8.1 W16-W23 S27-S24
13 1534 595 (S14W45 L=274) 629 97 0 (1486/ 562-1584/ 621) 45.0 W42-W47 S16-S11
14 1426 330 (S31W53 L=282) 379 64 0 (1395/ 314-1457/ 343) 45.0 W50-W54 S32-S29
15 1030 258 (S51W34 L=263) 1259 228 1 (1004/ 193-1062/ 337) -33.7 W27-W42 S55-S45
16 1342 286 (S37W51 L=280) 727 106 1 (1316/ 254-1374/ 325) -38.7 W46-W53 S39-S35
17 1077 255 (S49W37 L=266) 437 97 1 (1058/ 226-1102/ 294) -26.6 W33-W41 S51-S46
18 1182 256 (S45W43 L=273) 640 91 0 (1160/ 224-1205/ 293) -20.6 W39-W47 S46-S42
19 1107 184 (S53W47 L=276) 653 101 -1 (1062/ 165-1142/ 204) 14.0 W42-W50 S54-S51
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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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