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| 20140113 - Filament data for 08 UTC |
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Available data for 20140113: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1451 1438 (N24W26 L= 53) 1044 251 2 (1346/1381-1565/1515) -21.8 W19-W34 N20-N28
2 395 1483 (N22E47 L=340) 301 60 0 ( 381/1457- 410/1509) -53.1 E49-E45 N20-N24
3 1244 1453 (N23W12 L= 39) 541 104 1 (1186/1413-1297/1477) -23.2 W08-W15 N20-N24
4 331 1406 (N17E51 L=336) 353 66 0 ( 312/1369- 351/1437) 63.4 E51-E49 N15-N19
5 1092 1395 (N18W03 L= 29) 197 64 0 (1064/1365-1110/1413) -33.7 W00-W03 N16-N19
6 1279 1187 (N07W15 L= 41) 470 154 2 (1221/1144-1353/1253) -32.0 W10-W19 N04-N10
7 618 1186 (N04E26 L= 1) 200 84 1 ( 577/1168- 660/1200) 0.0 E28-E23 N02-N04
8 980 1118 (N01E03 L= 24) 303 117 0 ( 925/1076-1037/1149) 33.7 E06-W00 S01-N03
9 1926 1105 (N07W69 L= 96) 1713 273 2 (1892/1066-1968/1149) -15.3 W63-W78 N05-N09
10 441 1036 (S05E37 L=349) 755 137 1 ( 406/ 961- 476/1101) 63.4 E40-E34 S09-S01
11 1893 982 (S01W65 L= 92) 715 155 4 (1858/ 935-1924/1018) -26.6 W60-W70 S03-N01
12 812 939 (S10E13 L= 14) 422 238 0 ( 714/ 874- 915/ 983) 30.3 E18-E06 S14-S07
13 301 862 (S16E49 L=337) 700 185 1 ( 248/ 815- 369/ 903) 24.4 E54-E43 S18-S13
14 1824 726 (S16W61 L= 88) 5513 831 15 (1717/ 536-1945/ 896) 55.8 W49-W77 S29-S04
15 1826 844 (S10W59 L= 85) 546 90 3 (1795/ 818-1854/ 869) 19.4 W55-W62 S10-S07
16 986 615 (S30E01 L= 26) 2946 794 5 ( 694/ 455-1357/ 780) 27.1 E23-W22 S41-S17
17 731 709 (S25E18 L= 9) 301 88 1 ( 696/ 681- 768/ 742) 10.2 E20-E15 S26-S22
18 1709 707 (S19W50 L= 77) 297 49 1 (1684/ 683-1728/ 728) -56.3 W47-W51 S20-S17
19 332 593 (S33E51 L=335) 2445 466 12 ( 244/ 514- 441/ 642) -3.2 E59-E41 S37-S29
20 1293 423 (S41W25 L= 52) 666 82 0 (1247/ 391-1330/ 468) 71.6 W21-W27 S43-S37
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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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