|
|
|
|
| 20140127 - Filament data for 09 UTC |
|---|
|
Available data for 20140127: »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1573 1622 (N41W35 L=237) 330 67 1 (1558/1592-1591/1643) 68.2 W34-W37 N38-N43
2 294 1546 (N21E62 L=140) 685 210 1 ( 280/1493- 313/1600) -45.0 E66-E58 N17-N25
3 203 1335 (N07E65 L=137) 753 170 3 ( 160/1315- 243/1363) 5.2 E71-E59 N05-N08
4 736 1271 (N06E20 L=182) 198 70 1 ( 713/1247- 756/1313) 76.0 E21-E18 N04-N08
5 227 1143 (S05E57 L=145) 414 62 0 ( 204/1114- 247/1170) 36.9 E59-E55 S06-S03
6 1174 1056 (S02W08 L=210) 326 113 0 (1110/1022-1232/1078) -14.0 W04-W12 S03-S01
7 1295 953 (S07W17 L=219) 260 63 1 (1271/ 923-1327/ 990) -76.0 W15-W18 S08-S04
8 859 861 (S17E08 L=194) 306 116 1 ( 829/ 799- 890/ 914) 69.4 E09-E06 S21-S13
9 1424 861 (S10W26 L=228) 404 80 1 (1385/ 817-1461/ 910) 80.5 W24-W28 S12-S06
10 1266 844 (S13W17 L=219) 383 156 1 (1174/ 829-1333/ 867) 5.7 W11-W21 S14-S11
11 250 719 (S30E55 L=147) 2060 412 1 ( 197/ 603- 309/ 859) 48.8 E62-E47 S37-S21
12 1337 793 (S15W22 L=224) 196 34 1 (1315/ 776-1361/ 810) 45.0 W20-W23 S16-S14
13 1712 707 (S15W51 L=253) 2037 312 2 (1579/ 618-1830/ 799) 39.5 W42-W61 S21-S07
14 1001 700 (S25W02 L=204) 584 188 0 ( 922/ 635-1095/ 736) 38.7 E02-W08 S30-S22
15 1442 671 (S21W32 L=234) 486 164 1 (1368/ 623-1499/ 702) -18.4 W26-W35 S23-S19
16 1191 636 (S27W16 L=218) 424 111 1 (1133/ 606-1251/ 666) 35.5 W12-W19 S29-S24
17 1360 564 (S29W29 L=231) 794 200 0 (1285/ 525-1446/ 631) -4.4 W22-W35 S31-S25
18 1727 462 (S28W63 L=265) 1234 119 1 (1692/ 423-1766/ 505) 56.3 W60-W66 S31-S25
19 1368 314 (S46W42 L=244) 535 112 1 (1310/ 297-1422/ 343) 35.5 W37-W44 S47-S42
|
|
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.
|
|
|
|
