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| 20140401 - Filament data for 06 UTC |
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Available data for 20140401: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC »16 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 366 1593 (N10E64 L= 16) 2311 357 5 ( 300/1477- 421/1678) -77.9 E67-E58 N02-N16
2 444 1564 (N10E54 L= 26) 363 90 3 ( 419/1519- 470/1597) 90.0 E55-E52 N06-N12
3 1222 1368 (N18W02 L= 82) 683 267 0 (1203/1252-1255/1492) -61.7 E02-W06 N12-N26
4 1565 1380 (N30W23 L=103) 278 41 1 (1543/1359-1589/1403) -33.7 W21-W25 N29-N31
5 217 1311 (S09E65 L= 16) 1758 338 7 ( 164/1251- 273/1364) -54.5 E71-E57 S12-S05
6 735 1284 (N00E23 L= 57) 358 121 1 ( 678/1247- 801/1306) 0.0 E26-E18 S01-N01
7 1413 1236 (N16W16 L= 96) 386 137 0 (1393/1165-1430/1302) -54.5 W13-W18 N12-N19
8 857 1068 (S09E10 L= 70) 201 63 1 ( 831/1043- 894/1084) 33.7 E11-E08 S10-S07
9 1228 932 (S06W14 L= 94) 456 108 1 (1208/ 880-1247/ 991) -74.1 W12-W14 S09-S02
10 165 963 (S31E60 L= 21) 1577 427 3 ( 88/ 935- 241/ 988) 10.6 E68-E52 S32-S27
11 653 890 (S24E18 L= 62) 705 179 3 ( 591/ 823- 703/ 950) 68.2 E20-E15 S29-S19
12 1821 853 (N09W57 L=138) 635 108 3 (1801/ 810-1842/ 899) -51.3 W53-W61 N06-N11
13 410 763 (S38E34 L= 46) 1350 335 4 ( 308/ 728- 530/ 813) 21.8 E44-E24 S42-S33
14 1824 692 (N01W66 L=146) 1490 354 4 (1764/ 666-1897/ 748) 22.4 W59-W77 S02-N05
15 905 621 (S32W05 L= 86) 840 252 0 ( 825/ 542-1017/ 732) 76.8 W01-W08 S39-S22
16 1253 624 (S22W26 L=106) 540 179 1 (1164/ 572-1327/ 694) 65.6 W21-W27 S26-S15
17 1527 602 (S14W44 L=124) 305 129 1 (1481/ 576-1564/ 635) 0.0 W39-W47 S15-S12
18 1269 473 (S29W34 L=114) 272 59 0 (1237/ 460-1311/ 487) 31.0 W31-W36 S30-S27
19 1424 323 (S32W53 L=134) 426 44 1 (1393/ 308-1453/ 343) 36.9 W51-W55 S33-S30
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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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