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| 20140928 - Filament data for 10 UTC |
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Available data for 20140928: »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 1110 1706 (N44W32 L=250) 345 114 1 (1098/1668-1127/1753) 39.8 W28-W35 N41-N46
2 1230 1566 (N31W30 L=249) 618 182 2 (1149/1542-1317/1591) -20.0 W25-W36 N28-N33
3 1685 1505 (N13W60 L=278) 1926 406 5 (1622/1391-1780/1551) 0.0 W48-W72 N09-N14
4 452 1259 (N35E32 L=187) 309 75 0 ( 424/1224- 482/1300) 26.6 E34-E28 N32-N36
5 740 1278 (N29E10 L=208) 429 106 0 ( 678/1255- 797/1298) -29.7 E14-E06 N25-N30
6 1189 1244 (N14W15 L=234) 1905 452 4 ( 980/1198-1400/1279) -21.8 W02-W27 N08-N18
7 896 1238 (N22E02 L=217) 207 45 0 ( 878/1209- 915/1265) 56.3 E02-W00 N20-N23
8 417 1099 (N26E37 L=182) 989 237 2 ( 392/ 972- 440/1207) 81.9 E38-E34 N18-N32
9 1742 917 (S20W42 L=261) 1325 377 1 (1716/ 765-1767/1115) 63.4 W37-W49 S30-S09
10 792 903 (N06E16 L=202) 1079 296 2 ( 751/ 808- 863/1061) 70.3 E19-E10 N00-N14
11 1371 882 (S10W16 L=234) 221 48 2 (1355/ 848-1388/ 911) 76.0 W14-W17 S12-S08
12 1180 637 (S19E02 L=217) 2022 441 2 (1050/ 451-1258/ 798) 87.8 E06-W01 S32-S06
13 203 730 (N08E67 L=151) 670 120 1 ( 170/ 716- 240/ 752) -6.3 E73-E62 N06-N09
14 281 581 (S02E66 L=153) 609 133 3 ( 251/ 545- 314/ 614) -53.1 E70-E63 S04-N00
15 556 586 (S07E41 L=178) 295 82 1 ( 520/ 566- 595/ 600) -11.3 E43-E37 S07-S05
16 998 476 (S24E17 L=201) 334 123 1 ( 983/ 430-1022/ 531) 56.3 E19-E13 S27-S21
17 443 400 (S16E59 L=159) 729 219 1 ( 425/ 338- 462/ 452) 53.1 E63-E54 S20-S12
18 661 422 (S19E41 L=178) 403 81 0 ( 623/ 379- 695/ 452) -80.5 E42-E39 S22-S16
19 700 272 (S31E47 L=171) 931 231 1 ( 663/ 218- 723/ 332) 36.0 E53-E42 S34-S26
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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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