SDO HMI 2014-10-10 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.40 | 0.00 | 12.31 | -20.65 | 73.69 | 13.74 | 206.44 | 0.5099 | 238.9 | 80.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.66 | -23.24 | 83.49 | 23.54 | 217.22 | 0.6090 | 639.0 | 477.8 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -16.45 | 80.37 | 20.42 | 221.49 | 0.5072 | 470.0 | 354.0 | |
| 0.00 | 1.67 | 0.00 | 0.95 | -17.01 | 78.93 | 18.99 | 218.70 | 0.4996 | 703.0 | 541.9 | |
| 0.00 | 1.31 | 0.00 | 0.79 | -22.42 | 79.47 | 19.52 | 213.15 | 0.5672 | 590.0 | 549.9 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -16.83 | 76.68 | 16.73 | 215.48 | 0.4767 | 719.0 | 636.2 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -17.02 | 76.60 | 16.65 | 215.10 | 0.4784 | 746.0 | 640.3 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -17.40 | 76.37 | 16.42 | 214.26 | 0.4812 | 667.0 | 509.5 | |
| 0.00 | 1.84 | 0.00 | 1.04 | -17.50 | 76.15 | 16.20 | 213.79 | 0.4804 | 669.0 | 526.1 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -19.04 | 74.00 | 14.05 | 208.47 | 0.4834 | 687.0 | 492.6 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -18.47 | 73.72 | 13.78 | 208.60 | 0.4738 | 732.0 | 589.0 | |
| 0.00 | 3.77 | 0.00 | 2.17 | -23.33 | 68.49 | 8.54 | 195.51 | 0.5122 | -731.0 | -595.0 | |
| 0.00 | 1.67 | 0.00 | 0.96 | -23.67 | 68.28 | 8.33 | 194.96 | 0.5163 | -476.0 | -528.8 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -23.49 | 68.11 | 8.16 | 194.76 | 0.5131 | -809.0 | -701.9 | |
| 0.00 | 1.40 | 0.00 | 0.81 | -24.28 | 67.89 | 7.94 | 193.97 | 0.5237 | -509.0 | -402.5 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -23.90 | 67.47 | 7.52 | 193.45 | 0.5166 | -513.0 | -493.1 | |
| 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. | |