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| 20220515 - Latest Filament data |
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Available data for 20220515: »05 UTC »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
1 446 1602 (N19E58 L=111) 3399 399 8 ( 342/1520- 544/1684) 52.4 E67-E50 N13-N26
2 1647 1647 (N58W45 L=213) 683 65 1 (1631/1610-1671/1673) 31.6 W39-W55 N53-N61
3 363 1504 (N11E59 L=109) 987 141 1 ( 298/1466- 411/1546) 29.1 E66-E55 N08-N14
4 1582 1495 (N41W29 L=198) 342 54 1 (1563/1472-1606/1521) -33.7 W27-W31 N39-N42
5 581 1488 (N15E40 L=128) 282 72 1 ( 561/1453- 611/1511) 90.0 E41-E38 N12-N16
6 1695 1340 (N33W40 L=209) 481 70 1 (1671/1309-1718/1377) -45.0 W37-W42 N31-N35
7 175 1238 (S08E70 L= 99) 684 68 0 ( 140/1212- 209/1261) -4.4 E77-E63 S08-S06
8 150 929 (S27E69 L=100) 735 77 1 ( 130/ 894- 176/ 969) 39.8 E74-E64 S29-S24
9 868 721 (S24E02 L=166) 282 94 1 ( 846/ 679- 895/ 760) -78.7 E03-W00 S26-S21
10 781 669 (S29E07 L=162) 222 77 0 ( 739/ 648- 816/ 690) -9.5 E09-E03 S29-S28
11 1112 631 (S23W15 L=184) 246 76 1 (1071/ 610-1144/ 652) 11.3 W12-W17 S24-S22
12 1439 626 (S16W36 L=205) 248 58 0 (1410/ 600-1466/ 648) 63.4 W34-W37 S17-S13
13 1309 618 (S19W28 L=196) 246 51 0 (1293/ 587-1321/ 646) -45.0 W26-W29 S21-S17
14 322 586 (S47E51 L=118) 1251 145 2 ( 266/ 561- 390/ 628) 0.0 E59-E40 S49-S44
15 760 538 (S38E05 L=163) 291 48 0 ( 737/ 510- 784/ 562) 76.0 E06-E03 S40-S36
16 1553 372 (S27W62 L=230) 1346 163 2 (1502/ 328-1616/ 428) 83.7 W56-W65 S31-S22
17 1157 392 (S37W29 L=197) 455 82 1 (1114/ 369-1191/ 412) 0.0 W24-W32 S38-S35
18 779 376 (S50W01 L=169) 681 136 1 ( 754/ 317- 817/ 410) -40.6 E02-W05 S54-S46
19 794 278 (S59W07 L=176) 927 111 1 ( 747/ 245- 851/ 314) 29.1 W01-W10 S62-S53
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Download FITS filament maps as tar archive
» All Filament Data of 20220515 ...
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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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