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| 20140111 - Filament data for 07 UTC |
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Available data for 20140111: »07 UTC »08 UTC »09 UTC »10 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
1 372 1498 (N25E50 L= 4) 1759 373 4 ( 296/1414- 463/1570) -32.3 E60-E40 N18-N30
2 836 1473 (N23E14 L= 39) 248 38 0 ( 807/1458- 866/1491) -14.0 E16-E12 N22-N24
3 1082 1427 (N21W02 L= 56) 291 50 2 (1053/1405-1116/1450) -26.6 W00-W04 N19-N22
4 870 1361 (N16E11 L= 43) 313 126 1 ( 831/1304- 902/1414) -54.5 E13-E08 N12-N19
5 815 1217 (N07E13 L= 40) 369 125 1 ( 776/1168- 863/1274) -45.0 E16-E10 N03-N10
6 1735 1179 (N09W48 L=102) 402 130 3 (1699/1151-1770/1200) 23.2 W44-W51 N07-N10
7 548 1136 (N02E30 L= 23) 248 73 0 ( 514/1103- 586/1161) 21.8 E32-E27 N00-N03
8 1633 1063 (N01W39 L= 93) 577 80 2 (1599/1026-1672/1106) 63.4 W36-W42 S01-N03
9 1560 1073 (N01W34 L= 87) 408 95 1 (1518/1049-1596/1099) -9.5 W30-W36 N00-N02
10 1745 977 (S03W49 L=103) 519 136 1 (1703/ 950-1788/1003) -7.1 W45-W53 S04-S01
11 265 840 (S16E54 L=360) 511 170 1 ( 218/ 807- 299/ 896) 35.5 E58-E50 S18-S12
12 1759 754 (S16W54 L=107) 2893 732 12 (1659/ 666-1869/ 852) 42.5 W43-W66 S21-S09
13 1436 795 (S16W28 L= 81) 362 175 0 (1394/ 735-1488/ 851) 0.0 W24-W31 S19-S12
14 384 673 (S27E45 L= 8) 714 251 0 ( 328/ 598- 425/ 759) 45.0 E52-E40 S31-S21
15 595 603 (S32E29 L= 24) 2101 615 4 ( 426/ 448- 785/ 759) 32.9 E48-E14 S42-S20
16 1221 738 (S21W14 L= 67) 278 90 0 (1170/ 724-1269/ 756) 18.4 W10-W16 S21-S19
17 1472 652 (S25W32 L= 86) 790 149 2 (1435/ 588-1514/ 722) 83.7 W29-W34 S29-S20
18 1717 599 (S26W54 L=108) 1813 406 3 (1632/ 552-1831/ 686) 18.4 W47-W66 S29-S20
19 1501 478 (S36W40 L= 93) 566 91 1 (1451/ 444-1539/ 520) 45.0 W36-W42 S38-S33
20 979 467 (S40E01 L= 53) 225 40 2 ( 955/ 448-1005/ 484) 45.0 E02-W00 S41-S38
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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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