SOHO MDI 2000-07-11 17:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 173 | 1166 | 136 | 924 | -17.98 | 31.04 | 46.85 | 242.76 | 0.7791 | 180.6 | 63.4 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-11 17:35:31 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11 | 201 | 11 | 190 | -18.46 | 39.10 | 54.91 | 245.44 | 0.8554 | -598.4 | -207.6 | |
| 11 | -1 | 10 | -1 | -18.83 | 38.84 | 54.65 | 244.95 | 0.8543 | -851.3 | 999999 | |
| 7 | -1 | 6 | -1 | -18.29 | 38.45 | 54.25 | 245.42 | 0.8495 | -920.1 | 999999 | |
| 0 | 7 | 0 | 6 | -17.69 | 37.68 | 53.49 | 245.84 | 0.8414 | -663.0 | -529.7 | |
| 9 | 51 | 8 | 44 | -17.59 | 35.98 | 51.79 | 245.36 | 0.8262 | -746.8 | -466.0 | |
| 0 | 4 | 0 | 3 | -17.55 | 35.23 | 51.04 | 245.14 | 0.8193 | -140.0 | -302.5 | |
| 0 | 7 | 0 | 6 | -18.31 | 35.14 | 50.94 | 244.23 | 0.8208 | -701.0 | -591.1 | |
| 6 | 123 | 5 | 103 | -17.76 | 34.46 | 50.26 | 244.61 | 0.8129 | -607.3 | -653.0 | |
| 4 | -8 | 3 | -8 | -17.32 | 34.09 | 49.90 | 244.99 | 0.8080 | -997.8 | 999999 | |
| 8 | -8 | 7 | -8 | -17.69 | 33.91 | 49.72 | 244.48 | 0.8075 | -1059.6 | 999999 | |
| 6 | -8 | 5 | -8 | -17.83 | 33.38 | 49.19 | 244.11 | 0.8031 | -953.7 | 999999 | |
| 0 | 4 | 0 | 3 | -16.33 | 32.35 | 48.16 | 245.48 | 0.7880 | 446.0 | 252.8 | |
| 0 | 2 | 0 | 2 | -16.78 | 32.13 | 47.94 | 244.85 | 0.7875 | 290.0 | 127.0 | |
| 3 | 10 | 2 | 8 | -16.93 | 31.74 | 47.55 | 244.51 | 0.7843 | -844.1 | -657.5 | |
| 0 | 5 | 0 | 4 | -17.54 | 31.95 | 47.76 | 243.88 | 0.7885 | -249.0 | -373.3 | |
| 0 | 19 | 0 | 15 | -18.16 | 31.80 | 47.61 | 243.06 | 0.7894 | -731.0 | -399.5 | |
| 0 | 6 | 0 | 4 | -17.71 | 31.33 | 47.14 | 243.40 | 0.7832 | -843.0 | -658.7 | |
| 4 | 8 | 3 | 6 | -19.18 | 31.75 | 47.56 | 241.83 | 0.7928 | 60.9 | -36.7 | |
| 0 | 5 | 0 | 4 | -18.57 | 31.39 | 47.20 | 242.41 | 0.7870 | -366.0 | -411.5 | |
| 7 | 138 | 5 | 108 | -19.54 | 30.34 | 46.15 | 240.78 | 0.7809 | 631.1 | 94.3 | |
| 0 | 4 | 0 | 3 | -17.13 | 29.10 | 44.91 | 243.12 | 0.7587 | -367.0 | -478.9 | |
| 11 | -20 | 8 | -20 | -19.46 | 29.64 | 45.45 | 240.55 | 0.7739 | 1067.5 | 999999 | |
| 5 | 14 | 4 | 11 | -16.15 | 28.17 | 43.98 | 243.90 | 0.7450 | 560.0 | 401.4 | |
| 0 | 5 | 0 | 4 | -16.66 | 28.26 | 44.07 | 243.31 | 0.7481 | 603.0 | 361.3 | |
| 10 | -20 | 8 | -20 | -19.38 | 29.02 | 44.83 | 240.34 | 0.7676 | -484.1 | 999999 | |
| 0 | 7 | 0 | 5 | -15.96 | 27.66 | 43.47 | 243.91 | 0.7388 | -54.0 | 57.7 | |
| 0 | 4 | 0 | 3 | -17.44 | 27.86 | 43.67 | 242.14 | 0.7474 | -191.0 | -154.1 | |
| 3 | 10 | 2 | 7 | -16.93 | 27.65 | 43.46 | 242.68 | 0.7429 | 653.2 | 487.7 | |
| 25 | 201 | 18 | 144 | -16.15 | 26.36 | 42.17 | 243.03 | 0.7258 | 1441.7 | 646.1 | |
| 4 | 331 | 3 | 241 | -17.90 | 26.74 | 42.55 | 241.01 | 0.7379 | 756.8 | 409.9 | |
| -29 | -29 | -29 | -29 | -16.52 | 26.23 | 42.04 | 242.49 | 0.7262 | 999999 | 999999 | |
| 4 | -30 | 3 | -30 | -18.93 | 26.83 | 42.64 | 239.79 | 0.7437 | 717.9 | 999999 | |
| 6 | -30 | 4 | -30 | -18.19 | 26.60 | 42.41 | 240.58 | 0.7379 | 1045.5 | 999999 | |
| 8 | -29 | 6 | -29 | -17.11 | 26.17 | 41.98 | 241.71 | 0.7283 | 1280.1 | 999999 | |
| -29 | -29 | -29 | -29 | -16.25 | 25.94 | 41.75 | 242.69 | 0.7218 | 999999 | 999999 | |
| 5 | -30 | 3 | -30 | -18.48 | 26.40 | 42.21 | 240.12 | 0.7373 | 996.1 | 999999 | |
| 4 | -30 | 3 | -30 | -17.82 | 25.98 | 41.79 | 240.72 | 0.7297 | 1085.5 | 999999 | |
| 8 | -30 | 6 | -30 | -18.19 | 25.87 | 41.68 | 240.18 | 0.7304 | 1320.9 | 999999 | |
| 4 | -30 | 3 | -30 | -17.67 | 25.49 | 41.30 | 240.65 | 0.7238 | 1385.5 | 999999 | |
| 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. | |