SDO HMI 2014-05-25 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.89 | 348.22 | 94.87 | 435.37 | -18.57 | 149.57 | 65.73 | 250.30 | 0.9177 | 108.1 | 83.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.16 | 131.62 | 35.24 | 192.53 | -18.26 | 153.40 | 69.56 | 251.10 | 0.9421 | 487.7 | 75.7 | |
| 0.00 | 1.80 | 0.00 | 2.46 | -17.65 | 151.91 | 68.07 | 251.60 | 0.9331 | 554.0 | 457.0 | |
| 0.00 | 2.61 | 0.00 | 3.42 | -17.20 | 150.97 | 67.12 | 251.99 | 0.9271 | 710.0 | 523.9 | |
| 0.00 | 1.26 | 0.00 | 1.68 | -17.76 | 151.39 | 67.55 | 251.43 | 0.9301 | 636.0 | 554.6 | |
| 0.00 | 1.26 | 0.00 | 1.65 | -17.29 | 150.95 | 67.11 | 251.89 | 0.9271 | 469.0 | 535.6 | |
| 0.00 | 0.99 | 0.00 | 1.29 | -17.45 | 150.91 | 67.07 | 251.71 | 0.9269 | 642.0 | 568.3 | |
| 1.89 | 12.08 | 2.39 | 15.23 | -17.47 | 150.03 | 66.19 | 251.60 | 0.9213 | 187.9 | 376.9 | |
| 0.00 | 0.54 | 0.00 | 0.71 | -18.92 | 150.90 | 67.05 | 250.13 | 0.9278 | 461.0 | 478.3 | |
| 0.00 | 0.99 | 0.00 | 1.31 | -19.15 | 150.91 | 67.07 | 249.89 | 0.9281 | 454.0 | 454.1 | |
| 2.98 | 4.87 | 3.64 | 5.94 | -17.33 | 149.22 | 65.38 | 251.66 | 0.9160 | 658.5 | 522.3 | |
| 0.00 | 1.08 | 0.00 | 1.41 | -19.31 | 150.72 | 66.87 | 249.69 | 0.9270 | 524.0 | 534.5 | |
| 0.00 | 1.71 | 0.00 | 2.22 | -19.16 | 150.43 | 66.58 | 249.83 | 0.9251 | 419.0 | 489.8 | |
| 1.80 | 3.52 | 2.33 | 4.54 | -19.54 | 150.41 | 66.57 | 249.41 | 0.9253 | 523.4 | 417.2 | |
| 0.00 | 0.45 | 0.00 | 0.53 | -17.32 | 148.16 | 64.32 | 251.55 | 0.9087 | 474.0 | 490.2 | |
| 0.00 | 0.72 | 0.00 | 0.90 | -19.15 | 149.45 | 65.61 | 249.72 | 0.9189 | 323.0 | 358.8 | |
| 0.00 | 0.99 | 0.00 | 1.12 | -17.38 | 147.03 | 63.19 | 251.34 | 0.9008 | 186.0 | 128.9 | |
| 0.00 | 0.27 | 0.00 | 0.31 | -17.63 | 146.91 | 63.07 | 251.04 | 0.9002 | 125.0 | 169.7 | |
| 0.36 | 22.72 | 0.40 | 25.09 | -17.38 | 146.68 | 62.84 | 251.29 | 0.8983 | -258.8 | -377.6 | |
| 0.00 | 2.16 | 0.00 | 2.45 | -17.79 | 146.94 | 63.09 | 250.87 | 0.9005 | 327.0 | 323.7 | |
| 1.53 | -18.00 | 1.69 | -18.00 | -17.27 | 146.26 | 62.42 | 251.37 | 0.8951 | -480.1 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.93 | -19.10 | 147.23 | 63.39 | 249.48 | 0.9039 | -128.0 | -125.0 | |
| 0.00 | 1.98 | 0.00 | 2.23 | -18.75 | 146.71 | 62.87 | 249.78 | 0.8999 | 17.0 | 20.1 | |
| 9.20 | 143.79 | 10.10 | 156.45 | -17.94 | 146.05 | 62.20 | 250.59 | 0.8942 | -464.2 | 75.7 | |
| 6.40 | -23.00 | 6.96 | -23.00 | -17.69 | 145.76 | 61.92 | 250.82 | 0.8918 | -825.1 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.84 | -20.29 | 147.36 | 63.51 | 248.19 | 0.9060 | -324.0 | -293.8 | |
| 0.27 | -23.00 | 0.29 | -23.00 | -18.33 | 145.67 | 61.83 | 250.10 | 0.8918 | -395.0 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.31 | -20.93 | 147.33 | 63.49 | 247.48 | 0.9066 | -174.0 | -154.7 | |
| 0.81 | 4.87 | 0.91 | 5.43 | -19.98 | 146.35 | 62.50 | 248.37 | 0.8986 | -332.0 | -353.4 | |
| 0.99 | -28.00 | 1.10 | -28.00 | -19.79 | 146.21 | 62.37 | 248.56 | 0.8974 | -497.2 | 999999 | |
| 4.78 | -23.00 | 5.08 | -23.00 | -18.92 | 144.95 | 61.11 | 249.33 | 0.8871 | 787.6 | 999999 | |
| 0.00 | 2.16 | 0.00 | 2.27 | -18.41 | 144.65 | 60.80 | 249.85 | 0.8842 | 709.0 | 596.2 | |
| 2.07 | -23.00 | 2.24 | -23.00 | -19.62 | 145.27 | 61.42 | 248.60 | 0.8903 | -378.5 | 999999 | |
| 10.73 | -23.00 | 11.67 | -23.00 | -20.26 | 145.43 | 61.58 | 247.92 | 0.8923 | -559.9 | 999999 | |
| 9.92 | -23.00 | 10.83 | -23.00 | -20.68 | 145.44 | 61.60 | 247.45 | 0.8929 | 108.3 | 999999 | |
| 0.00 | 1.98 | 0.00 | 2.12 | -20.08 | 144.83 | 60.98 | 248.02 | 0.8876 | 147.0 | 137.5 | |
| 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. | |