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| 20240714 - Filament data for 08 UTC |
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Available data for 20240714: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 989 1680 (N49W00 L=169) 361 52 1 ( 968/1648-1016/1707) 68.2 E01-W02 N46-N51
2 1140 1664 (N47W14 L=183) 664 164 0 (1058/1639-1218/1684) -8.1 W06-W20 N44-N48
3 384 1568 (N41E59 L=110) 451 87 0 ( 348/1556- 433/1581) 5.2 E65-E52 N39-N41
4 1359 1500 (N33W27 L=196) 266 61 0 (1329/1477-1388/1522) -26.6 W25-W29 N31-N34
5 388 1343 (N25E47 L=122) 461 157 0 ( 340/1289- 424/1402) 58.0 E50-E43 N21-N29
6 696 1290 (N22E21 L=148) 586 159 1 ( 628/1245- 745/1325) -20.6 E25-E17 N18-N23
7 1406 1266 (N17W26 L=195) 399 144 0 (1355/1217-1447/1322) -54.5 W23-W28 N14-N21
8 517 1216 (N17E34 L=135) 254 63 1 ( 492/1190- 538/1248) 45.0 E35-E32 N15-N19
9 1201 953 (S01W11 L=179) 551 266 1 (1095/ 881-1303/ 998) -26.6 W04-W16 S05-N02
10 376 708 (S14E47 L=122) 1442 378 4 ( 338/ 554- 420/ 864) 63.4 E53-E40 S24-S04
11 1700 778 (S15W47 L=216) 424 109 2 (1650/ 742-1726/ 819) 38.7 W42-W49 S16-S12
12 974 664 (S18E05 L=164) 1405 328 6 ( 834/ 588-1060/ 728) -37.6 E13-W00 S23-S13
13 1665 607 (S26W47 L=216) 821 202 0 (1606/ 543-1718/ 685) 52.1 W43-W50 S30-S21
14 1292 599 (S24W16 L=185) 1270 270 3 (1203/ 502-1397/ 676) 37.6 W10-W23 S30-S19
15 512 312 (S44E56 L=113) 585 53 2 ( 488/ 295- 539/ 338) -71.6 E60-E52 S46-S41
16 1115 234 (S54W05 L=173) 454 74 0 (1098/ 209-1139/ 268) -63.4 W02-W07 S56-S50
17 1225 211 (S58W18 L=187) 838 87 1 (1192/ 179-1255/ 239) -45.0 W13-W22 S62-S53
18 1302 189 (S62W31 L=200) 1117 73 2 (1283/ 147-1321/ 232) -31.0 W24-W49 S70-S55
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Download FITS filament maps as tar archive
» All Filament Data of 20240714 ...
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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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