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| 20150108 - Latest Filament data |
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Available data for 20150108: »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 1517 1780 (N51W46 L=359) 588 155 0 (1507/1749-1529/1821) 53.1 W42-W51 N47-N55
2 1570 1694 (N43W45 L=357) 510 58 1 (1538/1669-1597/1717) -11.3 W42-W47 N40-N45
3 1640 1584 (N35W47 L=359) 445 77 0 (1609/1562-1672/1605) -26.6 W43-W49 N33-N36
4 910 1553 (N29E09 L=303) 295 93 0 ( 859/1533- 959/1567) -8.1 E12-E05 N27-N30
5 1713 1513 (N30W51 L= 3) 648 77 1 (1680/1479-1742/1541) -90.0 W47-W53 N27-N31
6 1012 1388 (N18E02 L=311) 447 98 0 ( 987/1333-1038/1437) -74.1 E03-W00 N14-N21
7 854 1271 (N11E11 L=301) 737 194 0 ( 749/1231- 946/1339) -22.6 E17-E05 N08-N14
8 415 1295 (N12E41 L=271) 656 166 2 ( 346/1243- 472/1334) 29.1 E45-E36 N09-N14
9 245 1290 (N12E56 L=256) 451 109 0 ( 209/1265- 282/1328) 26.6 E60-E52 N10-N14
10 312 1241 (N09E49 L=263) 964 161 2 ( 281/1165- 346/1325) 84.3 E51-E46 N04-N14
11 1866 1215 (N11W61 L= 14) 452 90 1 (1830/1196-1895/1229) -7.1 W57-W65 N10-N12
12 1556 1073 (N01W33 L=346) 403 79 2 (1524/1043-1599/1099) -11.3 W31-W36 S01-N02
13 1551 925 (S08W34 L=346) 876 270 2 (1477/ 818-1634/1028) 61.7 W29-W39 S14-S01
14 185 811 (S16E62 L=250) 4636 736 14 ( 107/ 719- 263/ 916) 42.7 E74-E53 S21-S09
15 323 833 (S15E48 L=264) 377 84 2 ( 288/ 810- 349/ 863) -9.5 E51-E45 S16-S13
16 789 665 (S26E15 L=297) 1175 301 2 ( 665/ 604- 858/ 786) 37.6 E23-E10 S30-S18
17 1431 701 (S22W28 L=340) 235 66 0 (1400/ 684-1452/ 733) 45.0 W25-W29 S23-S20
18 1673 616 (S26W48 L= 1) 719 157 1 (1606/ 557-1743/ 676) 41.6 W43-W53 S30-S22
19 1158 632 (S27W10 L=322) 425 72 1 (1122/ 595-1193/ 671) 78.7 W07-W11 S29-S24
20 1468 525 (S33W34 L=346) 473 99 0 (1410/ 491-1520/ 550) 29.7 W30-W37 S35-S31
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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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