|
|
|
|
| 20150421 - Filament data for 09 UTC |
|---|
|
Available data for 20150421: »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
1 989 1863 (N48E37 L=360) 485 51 1 ( 965/1845-1013/1885) 71.6 E40-E34 N45-N49
2 1024 1770 (N41E27 L= 10) 1340 272 1 ( 986/1694-1058/1838) -50.2 E32-E21 N34-N46
3 493 1584 (N14E51 L=346) 1434 418 3 ( 442/1449- 547/1695) -39.5 E61-E41 N06-N20
4 1084 1634 (N33E15 L= 22) 841 124 3 (1053/1583-1140/1693) -24.0 E19-E10 N29-N36
5 328 1535 (N07E65 L=332) 3093 417 5 ( 270/1467- 367/1614) -84.3 E73-E58 N02-N12
6 1707 1464 (N44W37 L= 74) 376 72 0 (1679/1449-1738/1481) 15.9 W33-W40 N42-N44
7 983 1261 (N07E09 L= 28) 326 86 0 ( 960/1222-1004/1321) -80.5 E09-E07 N04-N10
8 340 1222 (S11E49 L=348) 369 66 0 ( 316/1192- 363/1256) 63.4 E50-E47 S12-S08
9 1243 1052 (N02W11 L= 48) 295 110 1 (1186/1037-1304/1069) 33.7 W08-W14 N00-N04
10 1331 1040 (N04W17 L= 54) 216 17 0 (1312/1019-1348/1063) 90.0 W15-W17 N02-N05
11 1783 941 (N13W51 L= 88) 1856 314 2 (1715/ 817-1854/1009) 85.6 W44-W57 N05-N18
12 1818 842 (N08W58 L= 95) 1580 226 5 (1768/ 739-1860/ 961) -77.9 W53-W66 N01-N15
13 1690 873 (N06W45 L= 82) 313 48 1 (1671/ 843-1711/ 907) 78.7 W43-W46 N03-N08
14 1890 811 (N10W69 L=106) 595 88 0 (1876/ 766-1911/ 852) -78.7 W66-W70 N07-N12
15 491 820 (S31E28 L= 9) 266 56 0 ( 463/ 796- 514/ 844) 53.1 E30-E26 S32-S28
16 864 759 (S24E02 L= 35) 655 176 0 ( 777/ 733- 958/ 799) 45.0 E06-W02 S27-S19
17 1023 603 (S29W13 L= 50) 332 52 1 ( 987/ 582-1061/ 628) 11.3 W10-W15 S30-S27
18 792 541 (S40W00 L= 37) 496 123 0 ( 725/ 528- 853/ 555) 26.6 E04-W04 S41-S37
19 1295 232 (S42W52 L= 89) 555 63 0 (1259/ 217-1327/ 245) 36.9 W49-W54 S43-S40
|
|
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.
|
|
|
|
