|
|
|
|
| 20240802 - Filament data for 08 UTC |
|
Available data for 20240802: »07 UTC »08 UTC »09 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1464 1550 (N32W42 L=320) 1566 348 1 (1306/1487-1606/1590) -25.5 W30-W51 N25-N36
2 479 1533 (N45E41 L=237) 331 69 1 ( 452/1502- 502/1563) -32.0 E45-E37 N42-N47
3 328 1365 (N34E52 L=225) 1797 298 2 ( 215/1284- 422/1428) -16.9 E74-E40 N28-N38
4 930 1340 (N26E02 L=275) 496 217 0 ( 827/1329-1032/1350) -13.0 E09-W04 N24-N27
5 1568 1243 (N11W39 L=316) 793 234 3 (1533/1129-1607/1338) 85.6 W37-W41 N03-N16
6 1210 1149 (N11W13 L=290) 347 118 1 (1145/1130-1261/1168) -33.7 W09-W15 N09-N13
7 1823 1099 (S02W58 L=336) 1112 199 3 (1774/1048-1894/1151) 12.1 W53-W69 S04-N02
8 793 1045 (N10E14 L=264) 401 165 1 ( 777/ 969- 816/1119) 83.7 E14-E12 N05-N14
9 1838 951 (S11W59 L=336) 1151 147 4 (1776/ 899-1873/1020) 81.9 W51-W63 S15-S07
10 1725 846 (S15W46 L=324) 2219 385 6 (1685/ 713-1777/ 980) 86.6 W42-W51 S23-S06
11 1655 873 (S12W40 L=318) 729 187 2 (1620/ 803-1691/ 950) 66.0 W36-W43 S16-S07
12 331 777 (S03E51 L=226) 768 116 2 ( 301/ 742- 381/ 823) -45.0 E54-E47 S04-N00
13 1275 743 (S14W12 L=290) 305 74 0 (1235/ 728-1321/ 761) -18.4 W09-W15 S15-S13
14 251 690 (S08E63 L=215) 2762 204 6 ( 185/ 630- 331/ 755) -18.4 E73-E53 S12-S04
15 375 698 (S08E49 L=229) 800 147 2 ( 329/ 656- 411/ 741) -51.3 E52-E45 S10-S05
16 1195 605 (S22W06 L=283) 1600 368 2 (1145/ 506-1304/ 729) 82.4 W02-W12 S29-S14
17 338 542 (S18E60 L=218) 2598 217 7 ( 262/ 453- 379/ 627) 56.3 E67-E53 S24-S12
18 946 437 (S31E14 L=264) 406 95 1 ( 899/ 406- 983/ 474) 26.6 E17-E11 S32-S28
19 1374 377 (S43W18 L=296) 886 117 2 (1317/ 350-1424/ 412) 0.0 W13-W22 S45-S40
|
Download FITS filament maps as tar archive
» All Filament Data of 20240802 ...
|
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.
|
|
|
|