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| 20260210 - Filament data for 10 UTC |
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Available data for 20260210: »07 UTC »08 UTC »09 UTC »10 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 1178 1622 (N33E02 L=125) 453 78 1 (1145/1576-1207/1651) -45.0 E04-W00 N29-N35
2 1253 1584 (N32W04 L=131) 227 59 0 (1240/1553-1270/1615) -63.4 W02-W05 N29-N33
3 279 1490 (N11E63 L= 64) 3006 257 7 ( 213/1410- 352/1591) 69.0 E70-E58 N05-N18
4 1325 1561 (N32W09 L=136) 574 103 1 (1284/1526-1378/1591) 39.8 W06-W13 N28-N34
5 1417 1468 (N27W17 L=144) 477 105 1 (1381/1436-1461/1514) -23.2 W13-W20 N24-N30
6 1395 1126 (N06W20 L=147) 853 203 1 (1298/1071-1472/1180) -14.0 W13-W25 N04-N07
7 125 1142 (S11E71 L= 56) 1017 96 2 ( 77/1110- 164/1174) 7.1 E80-E64 S12-S09
8 1945 1077 (N17W69 L=196) 1760 136 5 (1914/ 998-1971/1132) -76.0 W64-W75 N12-N20
9 1885 1086 (N15W60 L=186) 559 74 1 (1871/1049-1900/1129) -63.4 W58-W62 N13-N17
10 563 1020 (S14E28 L= 99) 285 108 0 ( 524/ 984- 605/1064) 50.2 E30-E25 S16-S10
11 1729 1017 (N07W45 L=172) 325 91 1 (1715/ 968-1746/1055) -59.0 W43-W47 N04-N09
12 1888 992 (N10W61 L=188) 378 58 0 (1862/ 970-1907/1020) 38.7 W58-W63 N08-N12
13 734 954 (S15E16 L=111) 351 117 0 ( 672/ 930- 783/ 985) 26.6 E19-E13 S17-S13
14 1597 819 (S07W39 L=166) 352 86 2 (1551/ 801-1644/ 841) 26.6 W36-W42 S08-S04
15 654 700 (S32E19 L=108) 1539 409 1 ( 486/ 627- 850/ 772) 25.7 E32-E05 S39-S24
16 1150 667 (S25W15 L=142) 259 137 1 (1120/ 624-1199/ 711) -18.4 W12-W18 S26-S21
17 355 577 (S45E48 L= 79) 663 100 0 ( 312/ 531- 394/ 612) 26.6 E56-E42 S48-S41
18 1680 567 (S19W56 L=183) 454 76 1 (1661/ 541-1709/ 607) -26.6 W52-W59 S20-S16
19 1315 441 (S35W34 L=161) 1926 382 4 (1155/ 324-1459/ 530) 61.2 W28-W40 S46-S26
20 1745 449 (S23W73 L=200) 651 78 0 (1715/ 418-1781/ 470) 39.8 W70-W80 S25-S20
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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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