SDO HMI 2014-03-15 03:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.79 | 290.34 | 89.33 | 349.39 | 5.29 | 11.16 | 64.71 | 279.13 | 0.9134 | 174.6 | 29.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.04 | 7.39 | 1.64 | 11.58 | 5.02 | 17.19 | 70.74 | 277.74 | 0.9504 | -316.5 | -270.9 | |
| 6.78 | 9.12 | 9.16 | 12.33 | 6.19 | 13.76 | 67.31 | 279.59 | 0.9318 | -306.8 | -201.6 | |
| 0.00 | 3.13 | 0.00 | 4.21 | 6.60 | 13.56 | 67.11 | 280.05 | 0.9310 | -188.0 | -155.4 | |
| 15.73 | 266.53 | 19.41 | 316.09 | 3.53 | 12.01 | 65.56 | 277.07 | 0.9174 | -457.0 | 52.5 | |
| 0.00 | 3.04 | 0.00 | 3.80 | 6.69 | 11.78 | 65.33 | 280.51 | 0.9196 | -150.0 | -145.3 | |
| 4.00 | -4.00 | 4.86 | -4.00 | 5.09 | 11.34 | 64.89 | 278.88 | 0.9146 | 189.8 | 999999 | |
| 0.00 | 1.13 | 0.00 | 1.38 | 6.71 | 11.14 | 64.69 | 280.66 | 0.9153 | -162.0 | -140.1 | |
| 19.12 | -4.00 | 22.81 | -4.00 | 6.00 | 10.75 | 64.30 | 279.97 | 0.9117 | 440.6 | 999999 | |
| 1.39 | -4.00 | 1.63 | -4.00 | 5.10 | 10.36 | 63.91 | 279.08 | 0.9077 | 213.1 | 999999 | |
| 0.96 | -4.00 | 1.11 | -4.00 | 4.53 | 10.19 | 63.74 | 278.50 | 0.9057 | -425.9 | 999999 | |
| 2.78 | -4.00 | 3.25 | -4.00 | 5.43 | 10.29 | 63.84 | 279.45 | 0.9076 | 607.4 | 999999 | |
| 1.13 | -4.00 | 1.30 | -4.00 | 4.72 | 9.95 | 63.50 | 278.75 | 0.9042 | 478.6 | 999999 | |
| 3.48 | -4.00 | 3.98 | -4.00 | 4.53 | 9.85 | 63.40 | 278.56 | 0.9032 | 364.6 | 999999 | |
| 15.47 | -4.00 | 18.00 | -4.00 | 6.34 | 10.00 | 63.55 | 280.50 | 0.9068 | 691.1 | 999999 | |
| 1.91 | -4.00 | 2.18 | -4.00 | 4.97 | 9.73 | 63.28 | 279.06 | 0.9029 | 683.4 | 999999 | |
| 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. | |