SDO HMI 2010-11-16 18:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 136.18 | 663.07 | 91.72 | 447.11 | 13.73 | 172.58 | 41.51 | 287.75 | 0.6769 | -120.5 | -6.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.19 | 348.32 | 44.93 | 247.38 | 12.82 | 176.25 | 45.18 | 285.33 | 0.7195 | -1055.9 | -291.7 | |
| 0.26 | -1.00 | 0.18 | -1.00 | 12.82 | 175.35 | 44.28 | 285.53 | 0.7089 | -1084.0 | 999999 | |
| 7.73 | -1.00 | 5.36 | -1.00 | 12.65 | 174.88 | 43.82 | 285.39 | 0.7030 | -904.7 | 999999 | |
| 0.00 | 3.26 | 0.00 | 2.25 | 12.33 | 174.65 | 43.58 | 284.99 | 0.6995 | -730.0 | -626.5 | |
| 2.15 | -1.00 | 1.49 | -1.00 | 13.02 | 174.75 | 43.69 | 285.94 | 0.7022 | -808.4 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.88 | 11.20 | 174.01 | 42.94 | 283.52 | 0.6896 | -638.0 | -397.1 | |
| 0.00 | 0.43 | 0.00 | 0.29 | 10.92 | 173.63 | 42.56 | 283.17 | 0.6844 | -490.0 | -514.6 | |
| 0.00 | 1.37 | 0.00 | 0.94 | 12.72 | 173.81 | 42.74 | 285.73 | 0.6902 | -643.0 | -626.2 | |
| 0.00 | 0.86 | 0.00 | 0.58 | 12.09 | 173.48 | 42.41 | 284.91 | 0.6848 | -627.0 | -525.4 | |
| 0.00 | 0.77 | 0.00 | 0.52 | 11.99 | 173.00 | 41.94 | 284.87 | 0.6787 | -693.0 | -680.6 | |
| 0.00 | 0.60 | 0.00 | 0.40 | 12.11 | 173.03 | 41.96 | 285.04 | 0.6793 | -659.0 | -605.0 | |
| 0.00 | 2.83 | 0.00 | 1.91 | 12.62 | 173.09 | 42.02 | 285.77 | 0.6811 | -652.0 | -519.7 | |
| 0.00 | 1.12 | 0.00 | 0.75 | 11.90 | 172.78 | 41.72 | 284.80 | 0.6758 | -631.0 | -565.2 | |
| 1.20 | 2.40 | 0.81 | 1.62 | 13.08 | 172.85 | 41.79 | 286.49 | 0.6793 | 374.9 | 67.3 | |
| 0.00 | 6.70 | 0.00 | 4.47 | 13.18 | 172.35 | 41.28 | 286.78 | 0.6733 | 662.0 | 465.6 | |
| 0.00 | 0.86 | 0.00 | 0.57 | 15.31 | 171.27 | 40.21 | 290.23 | 0.6659 | 498.0 | 470.4 | |
| 0.00 | 0.52 | 0.00 | 0.34 | 15.77 | 171.26 | 40.19 | 290.90 | 0.6672 | 603.0 | 514.0 | |
| 0.69 | 5.32 | 0.45 | 3.46 | 13.54 | 170.38 | 39.31 | 287.90 | 0.6495 | -313.1 | -219.9 | |
| 1.20 | -18.00 | 0.78 | -18.00 | 13.73 | 170.25 | 39.19 | 288.22 | 0.6485 | -755.2 | 999999 | |
| 4.64 | 9.27 | 2.98 | 5.96 | 14.15 | 169.47 | 38.41 | 289.11 | 0.6398 | 674.0 | 539.0 | |
| 0.00 | 3.78 | 0.00 | 2.43 | 14.79 | 169.37 | 38.30 | 290.12 | 0.6406 | 399.0 | 461.4 | |
| 0.00 | 1.29 | 0.00 | 0.83 | 14.64 | 169.11 | 38.04 | 290.00 | 0.6368 | 571.0 | 475.8 | |
| 0.00 | 1.55 | 0.00 | 0.98 | 13.53 | 168.62 | 37.55 | 288.46 | 0.6270 | 544.0 | 453.8 | |
| 0.00 | 4.12 | 0.00 | 2.63 | 14.62 | 168.79 | 37.72 | 290.08 | 0.6327 | 630.0 | 575.3 | |
| 0.94 | 262.46 | 0.60 | 165.44 | 14.84 | 168.72 | 37.65 | 290.44 | 0.6325 | 616.8 | 390.4 | |
| 2.92 | -25.00 | 1.86 | -25.00 | 15.05 | 168.49 | 37.42 | 290.87 | 0.6303 | 666.8 | 999999 | |
| 1.55 | -25.00 | 0.98 | -25.00 | 14.81 | 168.44 | 37.37 | 290.51 | 0.6289 | 703.9 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.82 | 14.24 | 168.29 | 37.22 | 289.68 | 0.6250 | 548.0 | 358.1 | |
| 1.03 | -25.00 | 0.65 | -25.00 | 15.06 | 168.18 | 37.12 | 291.00 | 0.6265 | 862.8 | 999999 | |
| 1.20 | -25.00 | 0.76 | -25.00 | 14.91 | 168.15 | 37.09 | 290.78 | 0.6255 | 829.6 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.81 | 13.96 | 167.58 | 36.52 | 289.50 | 0.6149 | 630.0 | 487.3 | |
| 44.39 | -25.00 | 27.95 | -25.00 | 15.20 | 167.63 | 36.57 | 291.44 | 0.6200 | 1236.1 | 999999 | |
| 2.23 | -25.00 | 1.40 | -25.00 | 14.57 | 167.21 | 36.14 | 290.63 | 0.6122 | 857.2 | 999999 | |
| 0.86 | -25.00 | 0.54 | -25.00 | 15.64 | 167.26 | 36.20 | 292.28 | 0.6169 | 971.4 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.85 | 14.15 | 166.07 | 35.00 | 290.42 | 0.5958 | 838.0 | 685.4 | |
| 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. | |