SDO HMI 2014-07-10 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.89 | 93.11 | 28.48 | 113.08 | 14.19 | 261.61 | 66.04 | 283.83 | 0.9132 | -330.4 | -117.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.64 | 2.09 | 0.85 | 2.78 | 9.16 | 264.01 | 68.44 | 278.33 | 0.9296 | -358.4 | -287.6 | |
| 0.00 | 0.91 | 0.00 | 1.30 | 13.35 | 265.63 | 70.06 | 282.82 | 0.9395 | -307.0 | -251.2 | |
| 0.00 | 2.45 | 0.00 | 2.86 | 8.66 | 260.73 | 65.16 | 277.76 | 0.9072 | 302.0 | 246.5 | |
| 0.00 | 1.73 | 0.00 | 2.24 | 14.97 | 263.43 | 67.85 | 284.61 | 0.9263 | -155.0 | -152.5 | |
| 13.99 | 44.33 | 17.56 | 55.82 | 14.33 | 262.52 | 66.95 | 283.95 | 0.9203 | -525.8 | -119.1 | |
| 0.00 | 2.18 | 0.00 | 2.60 | 12.31 | 261.33 | 65.76 | 281.77 | 0.9117 | -534.0 | -431.1 | |
| 5.90 | 29.89 | 7.20 | 36.39 | 15.07 | 261.77 | 66.20 | 284.78 | 0.9154 | -478.0 | -235.2 | |
| 0.00 | 0.91 | 0.00 | 1.10 | 14.74 | 261.49 | 65.92 | 284.44 | 0.9134 | -453.0 | -421.8 | |
| 2.36 | -7.00 | 2.87 | -7.00 | 15.39 | 261.66 | 66.09 | 285.14 | 0.9148 | -582.6 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.71 | 17.35 | 260.69 | 65.12 | 287.35 | 0.9089 | 64.0 | 29.1 | |
| 0.00 | 1.54 | 0.00 | 1.39 | 11.19 | 252.27 | 56.70 | 280.87 | 0.8370 | 555.0 | 426.2 | |
| 0.00 | 1.64 | 0.00 | 1.48 | 11.72 | 252.32 | 56.75 | 281.49 | 0.8377 | 578.0 | 486.7 | |
| 0.00 | 1.54 | 0.00 | 1.36 | 9.60 | 251.38 | 55.81 | 279.00 | 0.8279 | 498.0 | 401.0 | |
| 0.00 | 1.36 | 0.00 | 1.18 | 11.42 | 250.89 | 55.32 | 281.23 | 0.8239 | 515.0 | 469.4 | |
| 0.00 | 1.09 | 0.00 | 0.87 | 16.29 | 246.35 | 50.78 | 287.82 | 0.7833 | 544.0 | 486.5 | |
| 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. | |