SDO HMI 2014-03-07 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.11 | 230.00 | 55.24 | 278.40 | -13.38 | 109.33 | 66.78 | 258.57 | 0.9120 | 375.9 | 208.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 1.83 | -14.97 | 117.53 | 74.99 | 256.47 | 0.9610 | 65.0 | 67.7 | |
| 5.62 | 22.49 | 9.70 | 38.85 | -15.44 | 117.17 | 74.63 | 255.99 | 0.9592 | 406.9 | 175.3 | |
| 2.68 | 4.41 | 3.70 | 6.09 | -11.22 | 112.49 | 69.94 | 260.72 | 0.9352 | 474.9 | 325.8 | |
| 0.00 | 0.52 | 0.00 | 0.82 | -16.72 | 115.52 | 72.98 | 254.73 | 0.9507 | 450.0 | 395.8 | |
| 0.43 | 1.47 | 0.65 | 2.20 | -16.02 | 114.44 | 71.89 | 255.52 | 0.9450 | -61.4 | 37.4 | |
| 0.00 | 0.95 | 0.00 | 1.31 | -18.15 | 112.67 | 70.13 | 253.29 | 0.9346 | 115.0 | 65.1 | |
| 4.50 | 12.28 | 6.33 | 17.16 | -18.93 | 113.22 | 70.68 | 252.45 | 0.9377 | -329.3 | -366.3 | |
| 5.54 | 20.93 | 6.54 | 24.73 | -12.79 | 108.70 | 66.16 | 259.22 | 0.9098 | -80.9 | 124.8 | |
| 0.43 | 2.16 | 0.58 | 2.90 | -18.43 | 112.10 | 69.55 | 253.00 | 0.9312 | -532.0 | -460.4 | |
| 0.00 | 1.04 | 0.00 | 1.21 | -13.31 | 108.37 | 65.82 | 258.66 | 0.9073 | -163.0 | -178.5 | |
| 0.00 | 0.61 | 0.00 | 0.74 | -15.88 | 109.76 | 67.21 | 255.80 | 0.9164 | 191.0 | 167.6 | |
| 24.39 | 159.07 | 27.15 | 177.14 | -12.31 | 107.00 | 64.45 | 259.82 | 0.8974 | 746.3 | 292.3 | |
| 0.00 | 1.99 | 0.00 | 2.23 | -14.91 | 107.24 | 64.70 | 256.92 | 0.8988 | -421.0 | -317.5 | |
| 0.52 | 1.04 | 0.59 | 1.19 | -16.09 | 107.88 | 65.33 | 255.59 | 0.9033 | -369.5 | -367.0 | |
| 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. | |