SDO HMI 2011-02-19 08:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 105.62 | 488.79 | 144.65 | 693.06 | -19.22 | 35.65 | 70.42 | 251.99 | 0.9355 | -17.1 | 78.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 1.70 | -17.08 | 39.02 | 73.79 | 254.23 | 0.9551 | 167.0 | 148.2 | |
| 0.69 | 1.80 | 1.11 | 2.91 | -17.37 | 38.66 | 73.43 | 253.94 | 0.9532 | 354.6 | 334.4 | |
| 6.18 | 192.18 | 10.68 | 316.05 | -18.50 | 39.95 | 74.72 | 252.72 | 0.9593 | -379.1 | 43.8 | |
| 12.02 | -3.00 | 20.31 | -3.00 | -18.52 | 39.50 | 74.27 | 252.71 | 0.9572 | 443.6 | 999999 | |
| 4.21 | -3.00 | 6.72 | -3.00 | -18.46 | 38.41 | 73.18 | 252.81 | 0.9518 | -377.2 | 999999 | |
| 13.57 | -3.00 | 21.20 | -3.00 | -18.48 | 37.99 | 72.76 | 252.80 | 0.9497 | 665.9 | 999999 | |
| 4.38 | 9.96 | 6.53 | 14.78 | -17.96 | 37.04 | 71.81 | 253.37 | 0.9447 | 450.3 | 444.6 | |
| 0.00 | 1.12 | 0.00 | 1.65 | -19.32 | 36.92 | 71.69 | 251.93 | 0.9439 | 473.0 | 361.2 | |
| 0.00 | 1.12 | 0.00 | 1.79 | -21.04 | 38.64 | 73.41 | 250.09 | 0.9527 | 335.0 | 269.5 | |
| 0.00 | 1.80 | 0.00 | 2.46 | -17.76 | 35.02 | 69.79 | 253.62 | 0.9331 | 356.0 | 303.7 | |
| 0.34 | 1.72 | 0.45 | 2.26 | -17.61 | 34.36 | 69.13 | 253.78 | 0.9291 | 167.0 | -116.2 | |
| 3.09 | 231.33 | 4.19 | 295.02 | -18.55 | 34.91 | 69.68 | 252.77 | 0.9324 | 691.8 | 132.6 | |
| 0.00 | 0.69 | 0.00 | 0.98 | -19.99 | 35.95 | 70.72 | 251.22 | 0.9385 | 426.0 | 337.9 | |
| 0.00 | 6.27 | 0.00 | 8.76 | -19.65 | 35.60 | 70.37 | 251.58 | 0.9365 | 459.0 | 476.0 | |
| 0.43 | -12.00 | 0.58 | -12.00 | -19.82 | 34.66 | 69.43 | 251.40 | 0.9309 | -218.6 | 999999 | |
| 1.12 | -12.00 | 1.50 | -12.00 | -19.98 | 34.63 | 69.40 | 251.23 | 0.9307 | -309.8 | 999999 | |
| 0.69 | -12.00 | 0.90 | -12.00 | -19.60 | 34.17 | 68.94 | 251.64 | 0.9279 | 330.4 | 999999 | |
| 3.09 | -12.00 | 4.05 | -12.00 | -19.94 | 34.14 | 68.91 | 251.27 | 0.9278 | 366.8 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.16 | -20.98 | 34.72 | 69.49 | 250.16 | 0.9313 | 329.0 | 343.9 | |
| 9.79 | -12.00 | 12.11 | -12.00 | -19.24 | 32.57 | 67.34 | 252.01 | 0.9178 | -529.2 | 999999 | |
| 2.66 | -12.00 | 3.32 | -12.00 | -19.69 | 32.79 | 67.56 | 251.53 | 0.9192 | -373.3 | 999999 | |
| 1.20 | -12.00 | 1.53 | -12.00 | -20.47 | 33.33 | 68.10 | 250.69 | 0.9228 | 234.2 | 999999 | |
| 1.55 | 2.15 | 1.84 | 2.55 | -18.60 | 31.57 | 66.34 | 252.70 | 0.9110 | -458.2 | -518.1 | |
| 2.32 | -12.00 | 2.93 | -12.00 | -20.43 | 33.13 | 67.90 | 250.72 | 0.9215 | -310.7 | 999999 | |
| 3.01 | -12.00 | 3.65 | -12.00 | -19.72 | 32.16 | 66.93 | 251.48 | 0.9151 | -790.1 | 999999 | |
| 10.30 | -12.00 | 12.61 | -12.00 | -20.11 | 32.33 | 67.11 | 251.06 | 0.9163 | -668.9 | 999999 | |
| 3.95 | -12.00 | 4.86 | -12.00 | -20.51 | 32.44 | 67.21 | 250.63 | 0.9171 | 740.3 | 999999 | |
| 0.00 | 1.89 | 0.00 | 2.24 | -19.28 | 31.40 | 66.17 | 251.96 | 0.9099 | -671.0 | -585.9 | |
| 0.00 | 3.61 | 0.00 | 4.29 | -19.48 | 31.56 | 66.33 | 251.74 | 0.9110 | -758.0 | -594.5 | |
| 3.18 | -12.00 | 3.89 | -12.00 | -20.90 | 32.30 | 67.07 | 250.20 | 0.9162 | 399.0 | 999999 | |
| 0.00 | 1.12 | 0.00 | 1.33 | -20.36 | 31.50 | 66.27 | 250.77 | 0.9108 | -517.0 | -399.1 | |
| 2.49 | 3.69 | 3.03 | 4.49 | -21.42 | 32.12 | 66.89 | 249.62 | 0.9152 | -521.3 | -511.6 | |
| 1.29 | 2.23 | 1.50 | 2.60 | -21.91 | 30.88 | 65.65 | 249.04 | 0.9070 | -198.9 | -175.4 | |
| 3.43 | 4.81 | 3.92 | 5.48 | -22.10 | 30.21 | 64.98 | 248.79 | 0.9024 | -430.2 | -327.9 | |
| 10.30 | 15.63 | 10.87 | 16.49 | -20.91 | 27.85 | 62.62 | 250.00 | 0.8847 | -663.9 | -513.4 | |
| 0.00 | 2.58 | 0.00 | 2.79 | -21.99 | 28.62 | 63.39 | 248.83 | 0.8910 | -653.0 | -476.8 | |
| 0.34 | 1.20 | 0.37 | 1.28 | -21.96 | 28.03 | 62.80 | 248.82 | 0.8866 | -623.5 | -557.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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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. |
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| 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. | |