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| 20140330 - Filament data for 14 UTC |
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Available data for 20140330: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC »16 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 568 1581 (N13E45 L= 57) 277 65 1 ( 545/1558- 582/1611) -76.0 E46-E43 N11-N15
2 317 1570 (N08E68 L= 34) 1226 160 3 ( 283/1531- 353/1602) 45.0 E73-E64 N05-N10
3 915 1515 (N18E20 L= 82) 704 196 1 ( 890/1426- 939/1602) -61.4 E23-E16 N12-N23
4 1290 1512 (N29W01 L=104) 604 114 2 (1260/1451-1317/1562) -45.0 E01-W04 N25-N31
5 1104 1372 (N15E05 L= 97) 617 174 0 (1075/1298-1121/1466) -56.3 E09-E03 N10-N19
6 518 1364 (S00E40 L= 63) 344 92 1 ( 487/1331- 557/1399) -15.9 E42-E35 S01-N01
7 892 1102 (S06E09 L= 93) 567 122 0 ( 853/1044- 916/1174) -76.0 E11-E07 S09-S01
8 308 916 (S31E45 L= 57) 3190 633 7 ( 153/ 761- 433/1101) 50.0 E60-E36 S42-S17
9 1669 981 (N10W40 L=142) 281 81 0 (1637/ 959-1690/1017) 90.0 W37-W40 N08-N12
10 1864 939 (N15W58 L=161) 495 61 1 (1842/ 910-1880/ 971) -76.0 W55-W60 N13-N17
11 1687 833 (N03W46 L=148) 1237 300 3 (1553/ 789-1808/ 883) 24.2 W34-W54 S01-N09
12 634 771 (S31E17 L= 85) 837 257 0 ( 563/ 676- 710/ 870) 68.2 E20-E13 S38-S23
13 970 789 (S21W04 L=106) 682 183 0 ( 877/ 731-1052/ 843) 61.4 W00-W06 S26-S15
14 1187 712 (S19W18 L=121) 514 114 0 (1126/ 673-1251/ 743) 54.5 W16-W21 S22-S15
15 1685 708 (S04W51 L=153) 386 69 1 (1654/ 674-1715/ 732) 59.0 W48-W52 S06-S01
16 1560 559 (S15W48 L=150) 417 74 1 (1522/ 534-1597/ 587) 45.0 W45-W49 S16-S12
17 1724 492 (S13W67 L=169) 527 146 4 (1703/ 467-1751/ 523) -14.0 W62-W71 S14-S10
18 1292 441 (S30W37 L=139) 1158 255 4 (1191/ 402-1404/ 477) 39.3 W31-W43 S34-S25
19 1541 411 (S23W55 L=158) 452 94 1 (1504/ 386-1577/ 443) 78.7 W52-W57 S25-S20
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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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