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| 20141123 - Filament data for 10 UTC |
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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 1619 1589 (N22W55 L=255) 1506 276 3 (1519/1551-1722/1645) -26.6 W48-W65 N18-N27
2 1700 1439 (N12W55 L=255) 696 159 1 (1632/1381-1742/1477) -53.1 W49-W57 N07-N15
3 1148 1419 (N22W16 L=216) 2186 557 7 ( 923/1379-1433/1445) -17.4 W01-W33 N16-N27
4 1254 1257 (N11W18 L=218) 362 135 0 (1188/1220-1300/1280) -45.0 W13-W20 N07-N12
5 1569 1254 (N04W38 L=238) 259 38 0 (1550/1233-1591/1275) 18.4 W36-W39 N03-N05
6 143 1209 (N29E62 L=138) 624 207 0 ( 112/1187- 182/1242) -26.6 E66-E57 N27-N31
7 707 1161 (N16E16 L=184) 668 165 0 ( 631/1096- 767/1213) -52.1 E20-E13 N10-N19
8 1833 1102 (S10W57 L=257) 863 199 2 (1788/1060-1889/1136) -10.3 W52-W63 S11-S08
9 212 1075 (N20E55 L=145) 460 73 3 ( 186/1041- 235/1105) -45.0 E57-E52 N17-N21
10 1796 1020 (S14W51 L=251) 1192 238 4 (1748/ 964-1853/1075) 24.4 W46-W57 S16-S11
11 1878 1010 (S16W60 L=259) 417 81 0 (1860/ 962-1893/1046) -80.5 W58-W61 S19-S13
12 1824 918 (S21W52 L=252) 919 182 2 (1790/ 837-1856/ 979) 69.4 W48-W56 S24-S16
13 1524 959 (S12W29 L=229) 264 99 1 (1477/ 936-1560/ 978) -26.6 W25-W31 S13-S10
14 286 897 (N08E51 L=149) 390 179 0 ( 229/ 882- 351/ 907) -10.3 E56-E45 N06-N09
15 300 611 (S09E59 L=141) 687 162 0 ( 287/ 550- 315/ 677) 53.1 E63-E56 S12-S04
16 251 616 (S08E65 L=135) 541 110 0 ( 237/ 573- 267/ 668) 63.4 E67-E62 S10-S04
17 1206 505 (S33W01 L=200) 903 219 0 (1100/ 443-1268/ 595) 23.2 E08-W06 S35-S28
18 638 505 (S21E36 L=164) 545 180 2 ( 586/ 451- 668/ 580) 31.0 E41-E31 S23-S16
19 749 404 (S30E33 L=167) 1140 267 2 ( 693/ 322- 809/ 498) 33.7 E40-E25 S34-S24
20 290 456 (S18E70 L=130) 860 75 0 ( 257/ 418- 319/ 489) -51.3 E72-E67 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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