SDO HMI 2011-06-18 14:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.98 | 160.35 | 45.26 | 146.74 | -14.80 | 245.93 | 55.47 | 251.32 | 0.8422 | 0.8 | 181.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 1.10 | -14.42 | 252.46 | 62.00 | 253.09 | 0.8956 | 154.0 | 109.0 | |
| 1.90 | 2.99 | 2.09 | 3.29 | -14.60 | 252.28 | 61.82 | 252.85 | 0.8945 | 263.1 | 226.2 | |
| 2.09 | 4.99 | 2.26 | 5.41 | -14.56 | 251.86 | 61.40 | 252.82 | 0.8913 | 509.0 | 440.9 | |
| 2.90 | 18.59 | 2.86 | 18.07 | -14.78 | 248.67 | 58.21 | 251.98 | 0.8663 | 401.5 | 401.1 | |
| 0.00 | 0.82 | 0.00 | 0.79 | -14.20 | 248.31 | 57.85 | 252.56 | 0.8623 | 224.0 | 205.8 | |
| 2.36 | -4.00 | 2.30 | -4.00 | -14.61 | 248.42 | 57.96 | 252.11 | 0.8639 | 316.3 | 999999 | |
| 0.00 | 2.18 | 0.00 | 2.10 | -14.23 | 248.08 | 57.62 | 252.49 | 0.8605 | 567.0 | 455.2 | |
| 3.63 | -4.00 | 3.51 | -4.00 | -14.64 | 248.08 | 57.62 | 252.02 | 0.8610 | 636.7 | 999999 | |
| 3.72 | -4.00 | 3.57 | -4.00 | -14.35 | 247.84 | 57.38 | 252.30 | 0.8586 | 638.0 | 999999 | |
| 2.99 | 5.53 | 2.81 | 5.19 | -13.92 | 247.09 | 56.63 | 252.63 | 0.8514 | 529.8 | 481.5 | |
| 0.00 | 1.00 | 0.00 | 0.94 | -14.14 | 247.00 | 56.54 | 252.36 | 0.8510 | 428.0 | 358.5 | |
| 0.00 | 0.91 | 0.00 | 0.87 | -15.70 | 247.35 | 56.89 | 250.64 | 0.8567 | 560.0 | 503.9 | |
| 1.45 | 36.55 | 1.35 | 33.71 | -14.57 | 246.54 | 56.08 | 251.76 | 0.8477 | 806.9 | 661.7 | |
| 1.45 | -13.00 | 1.34 | -13.00 | -14.76 | 246.45 | 55.99 | 251.52 | 0.8472 | 762.6 | 999999 | |
| 1.00 | 2.18 | 0.94 | 2.05 | -15.75 | 246.80 | 56.34 | 250.45 | 0.8521 | 424.7 | 403.7 | |
| 0.00 | 1.09 | 0.00 | 1.01 | -15.46 | 246.39 | 55.93 | 250.70 | 0.8480 | 491.0 | 458.2 | |
| 2.72 | 34.91 | 2.45 | 31.22 | -14.20 | 245.45 | 54.99 | 251.95 | 0.8372 | 332.5 | 130.7 | |
| 2.99 | -17.00 | 2.66 | -17.00 | -13.91 | 245.07 | 54.61 | 252.20 | 0.8332 | -406.8 | 999999 | |
| 2.18 | -17.00 | 1.92 | -17.00 | -13.72 | 244.79 | 54.33 | 252.37 | 0.8302 | -428.6 | 999999 | |
| 2.09 | -17.00 | 1.85 | -17.00 | -14.38 | 244.75 | 54.29 | 251.58 | 0.8311 | -350.8 | 999999 | |
| 0.00 | 1.81 | 0.00 | 1.62 | -14.82 | 244.91 | 54.45 | 251.09 | 0.8335 | -336.0 | -208.6 | |
| 0.00 | 2.09 | 0.00 | 1.84 | -14.00 | 244.61 | 54.15 | 252.00 | 0.8291 | -478.0 | -449.5 | |
| 0.00 | 2.54 | 0.00 | 2.25 | -15.01 | 244.71 | 54.25 | 250.82 | 0.8321 | -464.0 | -310.5 | |
| 0.00 | 1.00 | 0.00 | 0.87 | -14.65 | 244.25 | 53.79 | 251.13 | 0.8271 | -431.0 | -322.0 | |
| 0.00 | 1.63 | 0.00 | 1.45 | -16.15 | 244.50 | 54.04 | 249.43 | 0.8326 | -415.0 | -273.7 | |
| 0.00 | 1.36 | 0.00 | 1.17 | -14.32 | 243.39 | 52.93 | 251.32 | 0.8183 | -462.0 | -381.1 | |
| 0.00 | 0.73 | 0.00 | 0.63 | -15.69 | 243.52 | 53.06 | 249.72 | 0.8225 | -291.0 | -236.4 | |
| 2.09 | 2.63 | 1.82 | 2.29 | -16.64 | 243.57 | 53.11 | 248.60 | 0.8252 | -389.0 | -297.8 | |
| 9.79 | 20.40 | 8.45 | 17.56 | -16.19 | 243.23 | 52.77 | 249.04 | 0.8210 | -537.9 | -586.2 | |
| 0.00 | 1.09 | 0.00 | 0.92 | -14.59 | 242.50 | 52.04 | 250.77 | 0.8103 | -552.0 | -453.4 | |
| 1.18 | -29.00 | 1.01 | -29.00 | -16.09 | 242.93 | 52.47 | 249.08 | 0.8179 | -687.2 | 999999 | |
| 2.45 | 8.07 | 2.07 | 6.82 | -15.73 | 242.38 | 51.92 | 249.36 | 0.8118 | -714.2 | -587.1 | |
| 0.00 | 1.18 | 0.00 | 1.00 | -16.18 | 242.55 | 52.09 | 248.87 | 0.8145 | -579.0 | -498.0 | |
| 0.00 | 1.54 | 0.00 | 1.30 | -16.01 | 242.12 | 51.66 | 248.95 | 0.8100 | -679.0 | -520.2 | |
| 0.00 | 1.54 | 0.00 | 1.27 | -14.91 | 241.39 | 50.93 | 250.07 | 0.8002 | -613.0 | -541.1 | |
| 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. | |