| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 206 | 1719 | 111 | 919 | 17.03 | 308.76 | 18.41 | 306.64 | 0.3772 | 8.5 | 30.0 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-15 19:11:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 13 | 3 | 8 | 18.84 | 322.04 | 31.69 | 297.52 | 0.5628 | 912.5 | 680.1 | |
| 0 | 6 | 0 | 3 | 18.84 | 321.06 | 30.71 | 298.12 | 0.5502 | 613.0 | 695.3 | |
| 0 | 5 | 0 | 3 | 18.38 | 318.05 | 27.70 | 299.41 | 0.5084 | -613.0 | -496.0 | |
| 0 | 3 | 0 | 2 | 20.31 | 318.17 | 27.82 | 302.71 | 0.5223 | 436.0 | 581.7 | |
| 3 | 15 | 2 | 8 | 18.14 | 316.84 | 26.49 | 299.91 | 0.4910 | -939.1 | -847.1 | |
| 0 | 8 | 0 | 4 | 18.59 | 316.78 | 26.43 | 300.79 | 0.4930 | -835.0 | -589.6 | |
| 0 | 5 | 0 | 3 | 14.57 | 315.69 | 25.34 | 293.76 | 0.4544 | -636.0 | -501.7 | |
| 0 | 6 | 0 | 4 | 18.80 | 315.23 | 24.88 | 302.54 | 0.4744 | -842.0 | -879.6 | |
| 0 | 24 | 0 | 13 | 16.71 | 314.52 | 24.17 | 299.10 | 0.4506 | 1352.0 | 1019.4 | |
| 0 | 3 | 0 | 1 | 16.35 | 314.29 | 23.94 | 298.57 | 0.4452 | 673.0 | 691.9 | |
| 0 | 5 | 0 | 3 | 18.90 | 314.61 | 24.26 | 303.32 | 0.4670 | -756.0 | -646.1 | |
| 0 | 8 | 0 | 4 | 20.48 | 314.17 | 23.82 | 306.68 | 0.4736 | 666.0 | 538.4 | |
| 0 | 4 | 0 | 2 | 17.79 | 313.62 | 23.27 | 302.12 | 0.4460 | 358.0 | 306.5 | |
| 4 | 68 | 2 | 37 | 16.94 | 313.46 | 23.11 | 300.56 | 0.4379 | 1023.5 | 797.2 | |
| 0 | 5 | 0 | 3 | 24.23 | 314.34 | 23.99 | 312.85 | 0.5077 | -645.0 | -553.1 | |
| 11 | -14 | 6 | -14 | 17.03 | 313.03 | 22.68 | 301.18 | 0.4326 | 1301.2 | 999999 | |
| 0 | 7 | 0 | 4 | 18.26 | 313.01 | 22.66 | 303.68 | 0.4415 | 988.0 | 810.5 | |
| 4 | 34 | 2 | 19 | 17.07 | 311.91 | 21.56 | 302.41 | 0.4179 | 979.5 | 623.2 | |
| 20 | 108 | 11 | 58 | 15.14 | 311.47 | 21.12 | 298.63 | 0.3980 | -1696.8 | -608.6 | |
| 5 | -18 | 3 | -18 | 17.24 | 311.45 | 21.09 | 303.30 | 0.4130 | 724.7 | 999999 | |
| 0 | 4 | 0 | 2 | 15.75 | 311.27 | 20.92 | 300.23 | 0.3995 | -462.0 | -391.1 | |
| 16 | 39 | 8 | 21 | 14.60 | 310.50 | 20.15 | 298.40 | 0.3806 | -1494.3 | -863.7 | |
| 2 | 103 | 1 | 56 | 15.77 | 310.40 | 20.05 | 301.26 | 0.3876 | -1124.3 | 68.0 | |
| 2 | -23 | 1 | -23 | 17.02 | 310.45 | 20.10 | 304.01 | 0.3980 | 1057.2 | 999999 | |
| 0 | 7 | 0 | 4 | 17.83 | 310.54 | 20.19 | 305.63 | 0.4059 | 855.0 | 704.1 | |
| 10 | 29 | 5 | 16 | 19.24 | 310.09 | 19.74 | 309.08 | 0.4125 | 1231.0 | 796.9 | |
| 6 | 15 | 3 | 8 | 18.26 | 309.88 | 19.53 | 307.36 | 0.4011 | 854.4 | 577.5 | |
| 2 | 50 | 1 | 26 | 15.55 | 309.42 | 19.07 | 301.93 | 0.3724 | -1172.3 | -907.1 | |
| 0 | 5 | 0 | 2 | 17.98 | 309.67 | 19.32 | 307.04 | 0.3960 | 554.0 | 300.1 | |
| 5 | 25 | 3 | 13 | 19.33 | 309.39 | 19.04 | 310.22 | 0.4049 | 266.7 | -223.8 | |
| 1 | -28 | 1 | -28 | 15.40 | 308.97 | 18.62 | 302.13 | 0.3651 | -1060.8 | 999999 | |
| 12 | 752 | 7 | 401 | 17.22 | 309.02 | 18.67 | 306.28 | 0.3809 | -808.3 | 347.1 | |
| 3 | -30 | 2 | -30 | 19.63 | 309.20 | 18.85 | 311.06 | 0.4054 | -887.2 | 999999 | |
| 6 | -32 | 3 | -32 | 16.10 | 308.60 | 18.25 | 304.28 | 0.3657 | 318.5 | 999999 | |
| 0 | 8 | 0 | 4 | 14.33 | 308.40 | 18.05 | 300.20 | 0.3489 | -969.0 | -750.7 | |
| 0 | 11 | 0 | 6 | 13.85 | 308.23 | 17.88 | 299.17 | 0.3429 | -718.0 | -525.1 | |
| 6 | -32 | 3 | -32 | 15.95 | 308.20 | 17.85 | 304.47 | 0.3590 | -626.3 | 999999 | |
| 4 | -32 | 2 | -32 | 17.24 | 308.28 | 17.93 | 307.35 | 0.3715 | 1697.2 | 999999 | |
| 3 | -32 | 2 | -32 | 17.37 | 308.03 | 17.68 | 308.00 | 0.3694 | 1570.2 | 999999 | |
| 7 | -32 | 4 | -32 | 15.56 | 307.65 | 17.30 | 304.31 | 0.3482 | -978.8 | 999999 | |
| 4 | 14 | 2 | 7 | 14.07 | 307.48 | 17.13 | 300.73 | 0.3339 | -1213.2 | -945.4 | |
| 6 | -32 | 3 | -32 | 18.55 | 307.85 | 17.50 | 310.85 | 0.3785 | 1107.9 | 999999 | |
| 34 | -32 | 18 | -32 | 17.78 | 307.77 | 17.42 | 309.31 | 0.3700 | 1752.5 | 999999 | |
| -43 | -32 | -43 | -32 | 18.03 | 307.53 | 17.18 | 310.22 | 0.3694 | 999999 | 999999 | |
| 0 | 3 | 0 | 2 | 14.48 | 307.17 | 16.82 | 302.25 | 0.3327 | -1104.0 | -996.9 | |
| 0 | 8 | 0 | 4 | 16.10 | 306.66 | 16.31 | 307.14 | 0.3400 | -351.0 | -352.1 | |
| 0 | 4 | 0 | 2 | 13.13 | 306.44 | 16.09 | 299.60 | 0.3117 | -412.0 | -488.9 | |
| 4 | 13 | 2 | 7 | 21.21 | 306.78 | 16.43 | 317.79 | 0.3941 | 982.2 | 747.6 | |
| 0 | 5 | 0 | 3 | 20.67 | 306.67 | 16.32 | 316.97 | 0.3870 | 893.0 | 726.8 | |
| 0 | 23 | 0 | 12 | 14.54 | 305.94 | 15.59 | 304.30 | 0.3163 | -1123.0 | -945.5 | |
| 0 | 12 | 0 | 6 | 13.54 | 305.87 | 15.52 | 301.62 | 0.3069 | -1012.0 | -833.1 | |
| 0 | 9 | 0 | 5 | 13.91 | 305.73 | 15.38 | 302.88 | 0.3079 | -1128.0 | -962.3 | |
| 0 | 5 | 0 | 3 | 14.27 | 305.67 | 15.32 | 303.99 | 0.3101 | -979.0 | -780.9 | |
| 0 | 7 | 0 | 4 | 20.15 | 306.05 | 15.70 | 317.04 | 0.3743 | 893.0 | 799.3 | |
| 0 | 5 | 0 | 3 | 20.93 | 306.00 | 15.65 | 318.61 | 0.3826 | 828.0 | 658.9 | |
| 0 | 4 | 0 | 2 | 20.86 | 305.42 | 15.07 | 319.50 | 0.3757 | 559.0 | 455.8 | |
| 0 | 5 | 0 | 3 | 18.94 | 305.10 | 14.75 | 316.30 | 0.3501 | 675.0 | 574.1 | |
| 0 | 104 | 0 | 55 | 17.11 | 304.86 | 14.51 | 312.70 | 0.3273 | -1053.0 | -784.1 | |
| 0 | 7 | 0 | 4 | 21.13 | 304.48 | 14.13 | 321.72 | 0.3692 | 889.0 | 836.4 | |
| 0 | 5 | 0 | 2 | 18.18 | 304.05 | 13.70 | 316.72 | 0.3296 | -705.0 | -575.1 | |
| 0 | 5 | 0 | 2 | 22.21 | 304.06 | 13.71 | 324.40 | 0.3786 | 554.0 | 555.1 | |
| 0 | 10 | 0 | 5 | 18.32 | 303.12 | 12.77 | 318.96 | 0.3209 | -798.0 | -693.2 | |
| 20 | 92 | 11 | 48 | 16.75 | 302.16 | 11.81 | 317.52 | 0.2915 | -1690.3 | -808.1 | |
| 0 | 4 | 0 | 2 | 19.43 | 300.12 | 9.77 | 328.27 | 0.3057 | 778.0 | 615.3 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
||
| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |