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| 20140705 - Filament data for 08 UTC |
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Available data for 20140705: »07 UTC »08 UTC »09 UTC »10 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
1 595 1708 (N49E43 L=220) 393 70 1 ( 568/1688- 617/1722) -9.5 E46-E40 N47-N50
2 409 1268 (N17E43 L=220) 910 137 3 ( 364/1224- 442/1334) 81.9 E47-E40 N14-N21
3 934 1278 (N19E06 L=257) 255 51 1 ( 902/1259- 963/1294) -14.0 E08-E04 N17-N20
4 1088 1194 (N14W04 L=267) 585 212 1 (1018/1137-1145/1289) 60.9 W00-W07 N10-N19
5 917 1196 (N14E07 L=256) 502 202 1 ( 877/1130-1003/1282) -48.4 E09-E01 N09-N19
6 1862 1244 (N16W66 L=329) 553 105 2 (1844/1220-1884/1267) 36.9 W63-W69 N14-N17
7 1210 1104 (N08W11 L=275) 800 337 3 (1132/ 970-1258/1242) 69.4 W06-W14 N00-N16
8 214 1155 (N09E62 L=202) 1400 249 1 ( 173/1067- 236/1240) -51.3 E68-E58 N03-N13
9 983 862 (S07E02 L=261) 282 102 0 ( 953/ 828-1035/ 881) 14.0 E04-W00 S08-S05
10 1066 776 (S12W03 L=266) 250 37 1 (1041/ 750-1089/ 801) -33.7 W01-W04 S13-S10
11 1388 746 (S14W24 L=287) 722 100 2 (1355/ 693-1425/ 797) 63.4 W22-W26 S17-S10
12 301 706 (S19E53 L=210) 1350 236 5 ( 238/ 627- 350/ 795) -57.5 E58-E49 S24-S13
13 1099 717 (S16W05 L=268) 214 63 0 (1072/ 689-1127/ 753) 53.1 W03-W06 S17-S13
14 992 606 (S23E02 L=261) 572 185 1 ( 967/ 520-1015/ 674) 79.7 E03-W00 S29-S18
15 253 644 (S24E60 L=203) 929 208 3 ( 210/ 617- 298/ 668) 0.0 E65-E55 S25-S22
16 512 611 (S24E36 L=227) 302 112 0 ( 486/ 580- 541/ 656) 39.8 E38-E32 S26-S21
17 698 563 (S27E22 L=241) 428 116 0 ( 680/ 513- 724/ 608) 74.1 E23-E19 S30-S23
18 1262 560 (S26W17 L=280) 690 124 1 (1195/ 536-1306/ 597) 23.2 W12-W20 S28-S23
19 1051 487 (S32W03 L=266) 275 46 0 (1029/ 461-1072/ 515) 63.4 W01-W04 S33-S29
20 398 431 (S39E53 L=210) 598 115 1 ( 380/ 403- 417/ 466) 50.2 E56-E50 S41-S35
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Data will be available after one hour of observations. |
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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