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| 20141123 - Latest Filament data |
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Available data for 20141123: »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 1634 1594 (N22W57 L=255) 1559 263 1 (1536/1557-1729/1650) -28.1 W50-W66 N18-N27
2 1725 1436 (N11W57 L=255) 668 134 1 (1671/1376-1763/1471) -54.5 W53-W59 N07-N14
3 1164 1428 (N22W17 L=215) 2020 541 7 ( 937/1394-1443/1451) -15.7 W02-W35 N17-N27
4 1280 1264 (N11W20 L=218) 398 157 0 (1215/1228-1332/1290) -39.8 W15-W22 N07-N12
5 1593 1261 (N04W40 L=238) 375 48 0 (1563/1232-1619/1290) -45.0 W38-W41 N02-N06
6 1028 1239 (N14W04 L=203) 256 100 0 ( 994/1213-1074/1282) -59.0 W02-W06 N11-N17
7 159 1208 (N29E60 L=138) 508 137 0 ( 130/1191- 188/1227) -23.2 E63-E56 N27-N30
8 753 1140 (N14E14 L=185) 862 234 2 ( 654/1044- 829/1224) -63.4 E18-E10 N06-N20
9 1849 1112 (S10W59 L=257) 856 186 2 (1800/1078-1898/1141) -4.8 W53-W65 S11-S08
10 225 1088 (N20E54 L=145) 460 107 3 ( 196/1058- 258/1120) -53.1 E56-E50 N18-N22
11 1781 1024 (S13W50 L=248) 1641 358 6 (1701/ 928-1847/1100) -80.5 W43-W56 S19-S07
12 1840 925 (S20W54 L=253) 1018 157 2 (1808/ 846-1878/ 982) 69.4 W50-W58 S24-S16
13 311 903 (N08E49 L=150) 370 137 1 ( 260/ 885- 362/ 919) -6.3 E53-E44 N06-N08
14 1382 881 (S13W18 L=217) 202 69 0 (1361/ 864-1414/ 905) -33.7 W17-W20 S14-S11
15 261 625 (S07E63 L=135) 513 117 0 ( 249/ 580- 273/ 679) 56.3 E65-E60 S10-S04
16 314 607 (S09E58 L=140) 537 154 0 ( 300/ 549- 326/ 661) 40.6 E62-E55 S12-S06
17 1219 507 (S33W02 L=200) 895 213 0 (1114/ 449-1288/ 590) 21.0 E06-W07 S35-S29
18 765 411 (S30E32 L=167) 1117 256 1 ( 704/ 331- 830/ 504) 29.4 E39-E23 S34-S24
19 294 458 (S18E69 L=129) 1019 98 1 ( 259/ 420- 324/ 492) -59.0 E72-E66 S20-S15
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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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