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| 20150202 - Latest Filament data |
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Available data for 20150202: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 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
1 442 1570 (N21E49 L=293) 1329 284 4 ( 395/1465- 485/1637) -53.1 E55-E45 N13-N25
2 326 1598 (N22E62 L=280) 538 142 1 ( 301/1577- 350/1616) -23.2 E65-E58 N20-N23
3 560 1545 (N20E39 L=304) 642 91 0 ( 536/1508- 592/1589) -71.6 E40-E36 N17-N23
4 254 1525 (N17E67 L=275) 883 189 1 ( 233/1488- 283/1585) 71.6 E70-E63 N14-N21
5 1774 1492 (N37W51 L= 34) 508 144 0 (1750/1458-1802/1517) 40.6 W47-W55 N34-N40
6 484 1460 (N14E42 L=301) 317 59 1 ( 456/1441- 511/1492) 0.0 E43-E39 N12-N15
7 987 1456 (N19E08 L=334) 284 88 0 ( 946/1420-1013/1484) -31.0 E11-E06 N17-N20
8 353 1410 (N10E51 L=291) 432 91 0 ( 325/1373- 378/1459) 68.2 E53-E50 N07-N12
9 884 1396 (N14E14 L=329) 229 68 1 ( 846/1372- 911/1414) -11.3 E16-E11 N12-N15
10 874 1322 (N09E13 L=330) 211 59 1 ( 844/1295- 902/1342) -26.6 E15-E10 N08-N10
11 248 1095 (S10E54 L=288) 528 83 1 ( 227/1056- 269/1139) 90.0 E56-E52 S12-S07
12 102 1092 (S10E74 L=269) 720 108 3 ( 81/1065- 122/1131) 76.0 E77-E70 S11-S07
13 1162 1022 (S04W08 L=351) 192 74 0 (1121/ 988-1194/1056) -31.0 W05-W10 S05-S02
14 411 880 (S22E39 L=304) 1012 221 3 ( 332/ 834- 491/ 930) 24.8 E45-E32 S24-S18
15 1713 784 (S09W50 L= 32) 1134 242 2 (1679/ 687-1762/ 896) 90.0 W47-W53 S14-S01
16 1135 847 (S15W09 L=352) 314 94 0 (1098/ 817-1184/ 881) 51.3 W07-W11 S17-S12
17 1843 738 (S08W65 L= 47) 1307 244 4 (1799/ 694-1887/ 786) -26.6 W59-W72 S10-S05
18 1764 663 (S14W59 L= 41) 655 55 1 (1739/ 635-1792/ 692) 56.3 W56-W61 S16-S12
19 827 636 (S32E07 L=335) 436 78 2 ( 803/ 601- 854/ 675) -51.3 E09-E05 S34-S29
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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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