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| 20230704 - Filament data for 09 UTC |
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Available data for 20230704: »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
1 528 1649 (N43E50 L= 42) 461 44 0 ( 506/1625- 550/1678) -16.7 E55-E45 N41-N45
2 1410 1571 (N40W31 L=122) 388 64 0 (1378/1547-1439/1593) -31.0 W28-W33 N37-N41
3 297 1510 (N31E69 L= 22) 1047 158 0 ( 277/1441- 332/1574) -23.2 E79-E58 N26-N35
4 1679 1448 (N31W53 L=144) 729 148 1 (1636/1378-1717/1489) -63.4 W49-W56 N25-N33
5 1214 1369 (N25W12 L=104) 361 114 1 (1175/1329-1266/1401) 29.7 W09-W16 N22-N27
6 1490 1236 (N17W31 L=122) 871 337 1 (1383/1136-1612/1327) -38.7 W23-W39 N10-N22
7 1855 1262 (N18W68 L=160) 1272 98 1 (1829/1209-1875/1310) 71.6 W65-W72 N14-N20
8 1833 1185 (N13W63 L=154) 548 60 0 (1808/1158-1857/1208) -31.0 W59-W65 N11-N14
9 358 1151 (N08E47 L= 45) 385 161 0 ( 304/1089- 388/1189) -40.6 E52-E43 N04-N10
10 1749 856 (S07W52 L=144) 509 28 2 (1726/ 831-1772/ 880) 14.0 W50-W54 S08-S05
11 900 750 (S14E07 L= 84) 1191 280 3 ( 856/ 642- 945/ 876) 78.7 E10-E04 S21-S06
12 1042 839 (S08W02 L= 93) 280 150 1 (1003/ 819-1089/ 866) 26.6 W00-W04 S09-S06
13 451 785 (S14E39 L= 53) 266 70 1 ( 425/ 766- 488/ 806) 11.3 E40-E35 S15-S12
14 182 744 (S19E71 L= 20) 740 70 0 ( 153/ 721- 215/ 760) 9.5 E82-E64 S20-S17
15 1200 667 (S19W12 L=104) 377 103 1 (1165/ 626-1235/ 709) -45.0 W09-W15 S21-S16
16 1469 522 (S29W35 L=126) 1685 244 2 (1429/ 434-1521/ 640) -59.0 W31-W42 S35-S20
17 775 601 (S25E16 L= 75) 525 171 2 ( 691/ 585- 836/ 626) -11.3 E21-E11 S25-S22
18 1674 495 (S31W57 L=149) 571 88 1 (1632/ 483-1715/ 511) -9.5 W51-W63 S32-S29
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Download FITS filament maps as tar archive
» All Filament Data of 20230704 ...
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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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