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| 20150512 - Filament data for 08 UTC |
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Available data for 20150512: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 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
1 799 1834 (N43E46 L= 75) 444 106 0 ( 758/1816- 843/1848) 0.0 E50-E41 N42-N44
2 1359 1648 (N46W07 L=127) 1195 232 1 (1337/1564-1388/1732) -70.3 W03-W10 N39-N53
3 463 1651 (N22E58 L= 62) 1311 225 3 ( 408/1594- 497/1721) -78.7 E61-E54 N16-N26
4 888 1673 (N33E28 L= 92) 339 62 1 ( 868/1649- 912/1704) 90.0 E29-E26 N31-N36
5 546 1553 (N17E45 L= 75) 424 140 1 ( 523/1501- 578/1623) -66.0 E47-E42 N13-N22
6 1638 1584 (N51W35 L=156) 409 73 0 (1617/1562-1663/1602) 29.7 W32-W39 N48-N52
7 947 1562 (N27E19 L=101) 279 40 1 ( 919/1548- 978/1581) 14.0 E20-E16 N25-N28
8 633 1509 (N16E37 L= 83) 376 117 1 ( 604/1477- 670/1552) -23.2 E40-E33 N14-N18
9 712 1519 (N19E32 L= 88) 278 62 1 ( 687/1501- 740/1543) 71.6 E34-E30 N17-N20
10 971 1411 (N18E13 L=108) 796 254 2 ( 935/1313-1034/1508) -81.3 E15-E10 N12-N25
11 218 1206 (S10E61 L= 59) 973 138 3 ( 188/1157- 248/1260) -80.5 E64-E58 S12-S06
12 1275 1225 (N14W10 L=130) 380 65 2 (1240/1198-1308/1255) 26.6 W07-W11 N12-N16
13 285 1214 (S08E54 L= 66) 469 68 1 ( 259/1184- 315/1234) 18.4 E57-E51 S09-S06
14 1424 1106 (N11W22 L=142) 262 95 2 (1400/1061-1439/1157) -51.3 W19-W23 N08-N13
15 1106 1063 (N01W04 L=124) 251 45 2 (1080/1042-1132/1086) 45.0 W02-W05 N00-N02
16 1725 1001 (N13W46 L=166) 468 62 2 (1700/ 963-1750/1029) 63.4 W43-W47 N10-N14
17 621 770 (S27E19 L=101) 327 95 0 ( 578/ 752- 656/ 799) 38.7 E22-E17 S28-S24
18 798 575 (S35E03 L=117) 228 54 1 ( 776/ 557- 820/ 598) 45.0 E04-E01 S36-S33
19 1665 509 (S16W59 L=180) 930 200 2 (1627/ 464-1696/ 541) -63.4 W55-W63 S18-S14
20 1325 274 (S40W48 L=168) 917 179 1 (1251/ 260-1396/ 290) 15.3 W42-W54 S42-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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