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| 20140331 - Latest Filament data |
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Available data for 20140331: »06 UTC »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
1 341 1607 (N11E68 L= 22) 1741 281 4 ( 295/1548- 370/1665) -33.7 E74-E61 N07-N15
2 429 1564 (N10E55 L= 34) 671 107 1 ( 386/1537- 476/1595) 20.6 E60-E52 N07-N12
3 1089 1435 (N18E08 L= 82) 683 207 2 (1068/1340-1112/1536) -59.7 E11-E04 N12-N24
4 1457 1453 (N31W14 L=104) 454 72 2 (1430/1408-1479/1490) -59.0 W11-W15 N28-N33
5 1284 1300 (N16W07 L= 97) 531 155 1 (1254/1222-1305/1381) -58.0 W03-W09 N11-N19
6 687 1295 (S00E26 L= 63) 353 79 0 ( 653/1252- 730/1330) -8.1 E29-E22 S01-N01
7 180 1257 (S13E67 L= 23) 498 78 1 ( 156/1228- 199/1288) 53.1 E68-E64 S14-S10
8 1092 1011 (S05W04 L= 94) 304 63 0 (1070/ 975-1111/1053) -76.0 W03-W05 S07-S03
9 511 909 (S26E28 L= 61) 1173 214 3 ( 434/ 813- 574/1009) 71.6 E33-E25 S33-S18
10 864 957 (S15E07 L= 83) 183 84 1 ( 843/ 903- 885/ 994) -78.7 E08-E06 S17-S12
11 1756 886 (N08W50 L=139) 371 41 1 (1741/ 861-1773/ 913) 76.0 W47-W51 N06-N10
12 319 792 (S38E43 L= 47) 1510 295 3 ( 226/ 744- 427/ 837) 25.3 E52-E33 S43-S33
13 1807 747 (N03W60 L=150) 1196 343 1 (1704/ 716-1889/ 805) 24.0 W50-W68 N00-N09
14 786 688 (S32E05 L= 85) 926 283 0 ( 704/ 595- 879/ 794) 70.6 E07-E01 S40-S23
15 1137 694 (S21W16 L=106) 620 171 0 (1044/ 644-1208/ 759) 61.4 W12-W18 S26-S15
16 1402 677 (S14W32 L=122) 297 123 1 (1363/ 653-1454/ 716) 0.0 W28-W36 S15-S13
17 1781 645 (S03W63 L=153) 426 49 0 (1759/ 617-1804/ 671) 68.2 W61-W65 S05-N00
18 1179 539 (S29W25 L=115) 245 76 1 (1139/ 520-1221/ 560) 53.1 W22-W26 S30-S26
19 1641 484 (S16W59 L=149) 382 75 0 (1612/ 463-1676/ 501) 45.0 W56-W61 S17-S13
20 1408 351 (S31W50 L=140) 1732 270 2 (1306/ 314-1509/ 393) 45.0 W43-W56 S36-S25
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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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