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| 20240711 - Filament data for 09 UTC |
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Available data for 20240711: »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 1123 1618 (N43W10 L=218) 532 152 1 (1066/1568-1177/1660) -36.9 W05-W13 N38-N46
2 1228 1526 (N36W17 L=225) 252 39 1 (1211/1500-1242/1553) 53.1 W15-W18 N33-N37
3 1700 1484 (N30W58 L=266) 1279 146 0 (1634/1442-1768/1522) -21.0 W52-W66 N26-N32
4 262 1266 (N19E58 L=150) 1551 238 3 ( 227/1167- 313/1341) -65.6 E65-E53 N12-N23
5 1757 1266 (N16W55 L=263) 558 128 0 (1697/1233-1805/1285) -16.7 W49-W60 N13-N17
6 959 903 (S03E04 L=204) 219 83 0 ( 930/ 877- 979/ 942) 53.1 E06-E02 S04-N00
7 649 840 (S07E24 L=184) 907 255 1 ( 558/ 760- 734/ 927) -39.8 E30-E18 S11-S01
8 1125 760 (S13W06 L=214) 539 264 1 (1012/ 697-1163/ 829) 45.0 E01-W08 S16-S08
9 471 776 (S11E38 L=170) 312 65 0 ( 447/ 750- 494/ 810) 53.1 E39-E35 S12-S08
10 424 679 (S17E43 L=165) 3894 546 13 ( 268/ 560- 563/ 787) -30.6 E56-E33 S25-S10
11 1438 636 (S22W27 L=235) 666 228 1 (1338/ 570-1491/ 700) 35.0 W20-W30 S26-S17
12 712 595 (S23E22 L=186) 1077 288 1 ( 652/ 468- 784/ 687) 51.3 E29-E16 S31-S16
13 1309 607 (S23W18 L=226) 523 112 0 (1269/ 572-1359/ 643) 33.7 W15-W21 S25-S20
14 1120 541 (S27W05 L=213) 320 98 0 (1088/ 505-1158/ 582) 51.3 W03-W07 S29-S24
15 1181 403 (S38W11 L=218) 1382 349 4 (1077/ 318-1314/ 489) 37.4 W02-W19 S45-S31
16 745 418 (S36E23 L=185) 456 63 1 ( 708/ 399- 778/ 447) 18.4 E26-E20 S37-S33
17 628 393 (S38E35 L=173) 426 77 1 ( 600/ 364- 656/ 426) -78.7 E36-E31 S40-S35
18 1009 347 (S42E03 L=205) 590 85 1 ( 966/ 323-1041/ 373) -33.7 E06-W00 S44-S39
19 911 193 (S58E17 L=191) 521 50 1 ( 893/ 172- 935/ 221) -80.5 E20-E14 S61-S54
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Download FITS filament maps as tar archive
» All Filament Data of 20240711 ...
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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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