| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 386 | 2775 | 378 | 2775 | 10.66 | 77.42 | -60.95 | 81.75 | 0.8680 | 364.8 | 106.7 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-09-19 17:50:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 2078 | 11 | 1948 | 11.14 | 82.74 | -55.63 | 81.35 | 0.8214 | 1250.3 | 215.6 | |
| 84 | -1 | 73 | -1 | 9.79 | 82.26 | -56.12 | 82.98 | 0.8265 | 1393.8 | 999999 | |
| 0 | 3 | 0 | 3 | 7.35 | 82.73 | -55.65 | 85.97 | 0.8230 | 173.0 | 83.8 | |
| 31 | -1 | 28 | -1 | 9.70 | 81.41 | -56.96 | 83.05 | 0.8346 | 756.4 | 999999 | |
| 0 | 12 | 0 | 11 | 5.56 | 82.11 | -56.26 | 88.08 | 0.8303 | -535.0 | -364.8 | |
| 3 | -1 | 2 | -1 | 9.53 | 80.87 | -57.51 | 83.23 | 0.8398 | 12.3 | 999999 | |
| 18 | -1 | 16 | -1 | 12.08 | 79.93 | -58.44 | 80.17 | 0.8478 | -436.7 | 999999 | |
| 12 | -1 | 11 | -1 | 10.35 | 80.41 | -57.96 | 82.23 | 0.8438 | 863.8 | 999999 | |
| 6 | -1 | 5 | -1 | 10.96 | 79.84 | -58.53 | 81.49 | 0.8488 | 819.3 | 999999 | |
| 4 | 13 | 4 | 12 | 6.26 | 80.92 | -57.46 | 87.13 | 0.8412 | 1.7 | 88.1 | |
| 12 | -1 | 12 | -1 | 10.33 | 79.50 | -58.87 | 82.22 | 0.8521 | 805.9 | 999999 | |
| 9 | -1 | 8 | -1 | 11.30 | 78.88 | -59.50 | 81.06 | 0.8574 | 786.2 | 999999 | |
| 8 | -1 | 8 | -1 | 9.30 | 79.49 | -58.89 | 83.43 | 0.8526 | 360.4 | 999999 | |
| 43 | -1 | 41 | -1 | 10.55 | 78.57 | -59.81 | 81.92 | 0.8603 | 762.4 | 999999 | |
| 5 | -1 | 5 | -1 | 11.71 | 77.93 | -60.45 | 80.55 | 0.8655 | 631.1 | 999999 | |
| 10 | -1 | 11 | -1 | 14.68 | 76.57 | -61.80 | 77.12 | 0.8766 | -482.7 | 999999 | |
| 3 | -1 | 3 | -1 | 11.17 | 76.97 | -61.41 | 81.14 | 0.8738 | 501.8 | 999999 | |
| 15 | -1 | 15 | -1 | 11.64 | 76.54 | -61.84 | 80.59 | 0.8772 | 449.5 | 999999 | |
| 17 | -1 | 17 | -1 | 9.94 | 76.97 | -61.40 | 82.55 | 0.8742 | -568.4 | 999999 | |
| 6 | 149 | 7 | 160 | 14.22 | 74.94 | -63.43 | 77.62 | 0.8895 | 163.3 | 5.1 | |
| 13 | -1 | 13 | -1 | 9.31 | 76.58 | -61.79 | 83.26 | 0.8777 | -687.1 | 999999 | |
| 4 | -20 | 4 | -20 | 13.06 | 74.88 | -63.50 | 78.94 | 0.8902 | 307.2 | 999999 | |
| 14 | -1 | 15 | -1 | 10.39 | 75.27 | -63.11 | 81.95 | 0.8879 | -762.5 | 999999 | |
| 0 | 4 | 0 | 5 | 11.91 | 73.55 | -64.82 | 80.17 | 0.9005 | -299.0 | -292.4 | |
| 6 | 90 | 6 | 101 | 8.16 | 74.03 | -64.35 | 84.38 | 0.8985 | -755.2 | -500.6 | |
| 0 | 9 | 0 | 10 | 12.90 | 71.99 | -66.38 | 79.03 | 0.9115 | -552.0 | -516.8 | |
| 6 | -25 | 7 | -25 | 7.75 | 73.87 | -64.51 | 84.83 | 0.8999 | -673.6 | 999999 | |
| 8 | 97 | 10 | 122 | 14.24 | 70.38 | -68.00 | 77.50 | 0.9222 | -668.9 | -286.9 | |
| 2 | 14 | 2 | 17 | 10.39 | 72.37 | -66.00 | 81.80 | 0.9096 | -572.4 | -466.6 | |
| 0 | 4 | 0 | 5 | 9.90 | 72.57 | -65.80 | 82.35 | 0.9084 | -424.0 | -352.2 | |
| 2 | -28 | 3 | -28 | 13.93 | 70.46 | -67.91 | 77.85 | 0.9217 | -585.0 | 999999 | |
| 3 | -28 | 4 | -28 | 13.15 | 70.71 | -67.67 | 78.70 | 0.9202 | -433.2 | 999999 | |
| 0 | 54 | 0 | 63 | 8.70 | 72.52 | -65.85 | 83.67 | 0.9093 | -617.0 | -533.0 | |
| 3 | 61 | 4 | 84 | 14.48 | 68.63 | -69.75 | 77.18 | 0.9332 | -411.8 | -12.9 | |
| 4 | 177 | 5 | 221 | 8.78 | 71.50 | -66.88 | 83.50 | 0.9165 | -571.4 | 49.4 | |
| 4 | -34 | 5 | -34 | 14.68 | 68.25 | -70.13 | 76.95 | 0.9354 | -265.3 | 999999 | |
| 7 | -35 | 8 | -35 | 8.41 | 71.33 | -67.05 | 83.90 | 0.9178 | -426.4 | 999999 | |
| 12 | -35 | 15 | -35 | 9.05 | 70.67 | -67.70 | 83.15 | 0.9220 | -218.0 | 999999 | |
| 0 | 10 | 0 | 13 | 10.40 | 69.65 | -68.72 | 81.62 | 0.9280 | 359.0 | 275.3 | |
| 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. | |