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| 20150420 - Filament data for 08 UTC |
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Available data for 20150420: »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
1 901 1773 (N37E35 L= 16) 2929 528 3 ( 858/1649- 970/1929) -37.2 E54-E23 N28-N50
2 397 1502 (N06E55 L=355) 547 142 0 ( 383/1443- 412/1562) -58.0 E59-E52 N02-N10
3 1605 1511 (N43W26 L= 77) 358 65 1 (1583/1481-1627/1530) -56.3 W23-W28 N40-N44
4 1775 1387 (N40W44 L= 94) 2216 341 4 (1651/1309-1861/1477) -5.0 W30-W54 N36-N43
5 1349 1409 (N26W08 L= 59) 298 110 0 (1319/1347-1366/1452) -56.3 W05-W09 N21-N28
6 777 1346 (N06E23 L= 28) 439 48 1 ( 748/1308- 803/1382) -63.4 E24-E21 N04-N08
7 1846 1253 (N34W51 L=102) 807 154 1 (1804/1217-1873/1283) 32.0 W46-W54 N31-N36
8 1128 1143 (N04W03 L= 53) 199 19 0 (1110/1123-1145/1166) 90.0 W01-W03 N02-N05
9 1037 1154 (N02E03 L= 48) 248 115 0 ( 978/1139-1099/1165) 31.0 E05-W00 N00-N03
10 1665 1037 (N14W38 L= 89) 787 212 0 (1629/ 963-1718/1086) 76.0 W35-W42 N09-N17
11 1578 1030 (N11W32 L= 83) 463 112 1 (1545/ 983-1607/1084) -51.3 W28-W34 N07-N13
12 416 1035 (S20E38 L= 13) 259 70 0 ( 401/ 992- 431/1072) -53.1 E39-E36 S22-S18
13 833 949 (S14E09 L= 42) 248 62 2 ( 818/ 908- 855/ 987) -76.0 E09-E07 S16-S12
14 1691 896 (N07W44 L= 95) 788 151 1 (1640/ 835-1729/ 957) 77.5 W41-W48 N02-N11
15 1829 894 (N12W57 L=108) 569 97 4 (1805/ 854-1857/ 939) 80.5 W54-W59 N08-N14
16 378 895 (S29E39 L= 12) 671 171 2 ( 313/ 847- 439/ 938) 41.6 E44-E34 S33-S25
17 685 856 (S24E15 L= 35) 589 195 0 ( 603/ 823- 779/ 903) 42.0 E20-E10 S27-S18
18 859 703 (S28E01 L= 50) 440 104 2 ( 826/ 671- 891/ 736) 76.0 E02-W01 S29-S25
19 642 628 (S39E13 L= 38) 461 68 1 ( 607/ 612- 688/ 653) 8.1 E16-E09 S40-S37
20 1178 301 (S42W39 L= 90) 306 47 0 (1152/ 280-1203/ 319) 0.0 W36-W41 S42-S41
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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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