|
|
|
|
| 20240717 - Filament data for 08 UTC |
|
Available data for 20240717: »06 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 1481 1727 (N48W55 L=184) 448 58 0 (1457/1702-1503/1752) 16.7 W50-W60 N46-N49
2 877 1420 (N30E08 L=121) 648 183 1 ( 813/1350- 912/1498) -59.0 E13-E05 N25-N35
3 1279 1336 (N22W19 L=148) 736 243 0 (1203/1243-1344/1371) -45.0 W13-W22 N16-N24
4 243 1293 (N23E61 L= 68) 1083 122 2 ( 217/1236- 272/1352) -60.3 E63-E57 N19-N26
5 1816 1270 (N13W63 L=191) 544 75 3 (1785/1236-1839/1302) -76.0 W59-W65 N11-N15
6 388 1284 (N23E45 L= 84) 283 62 1 ( 356/1265- 419/1297) 0.0 E48-E42 N21-N23
7 176 1239 (N19E70 L= 59) 1112 108 1 ( 153/1187- 196/1286) 66.8 E73-E66 N15-N22
8 1554 1197 (N12W36 L=165) 341 76 2 (1530/1167-1587/1228) -45.0 W34-W38 N09-N13
9 1835 939 (S07W60 L=188) 590 70 2 (1821/ 904-1856/ 978) -68.2 W57-W62 S09-S04
10 1634 839 (S11W40 L=169) 505 93 1 (1611/ 788-1658/ 889) 63.4 W38-W42 S14-S07
11 1569 837 (S10W35 L=164) 282 63 4 (1534/ 816-1602/ 858) 0.0 W32-W37 S11-S09
12 1538 754 (S16W33 L=162) 802 232 5 (1423/ 709-1602/ 816) -8.7 W24-W37 S18-S11
13 950 741 (S13E06 L=123) 470 201 0 ( 904/ 661-1016/ 811) 48.4 E09-E01 S17-S08
14 485 734 (S12E38 L= 91) 304 92 3 ( 462/ 684- 508/ 766) 51.3 E39-E35 S14-S09
15 1797 691 (S23W59 L=188) 1137 130 1 (1748/ 657-1843/ 736) 16.7 W53-W65 S24-S20
16 1539 670 (S21W34 L=162) 525 136 2 (1480/ 647-1585/ 697) -7.1 W29-W37 S22-S19
17 1512 602 (S26W32 L=161) 365 89 2 (1483/ 571-1535/ 633) -45.0 W29-W34 S27-S23
18 595 533 (S25E33 L= 95) 1097 145 3 ( 570/ 459- 641/ 600) 59.0 E37-E30 S30-S20
19 484 433 (S33E48 L= 81) 1001 175 2 ( 408/ 414- 569/ 454) -3.6 E56-E39 S34-S31
|
Download FITS filament maps as tar archive
» All Filament Data of 20240717 ...
|
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.
|
|
|
|