SDO HMI 2014-09-13 17:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.44 | 25.27 | 0.27 | 15.61 | -22.95 | 73.52 | 20.54 | 212.95 | 0.5985 | 39.8 | -4.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.58 | -21.06 | 81.93 | 28.95 | 224.54 | 0.6463 | 698.0 | 503.2 | |
| 0.00 | 1.24 | 0.00 | 0.75 | -14.15 | 80.64 | 27.66 | 232.10 | 0.5727 | 625.0 | 502.7 | |
| 0.00 | 1.16 | 0.00 | 0.74 | -21.55 | 80.01 | 27.03 | 222.06 | 0.6333 | 773.0 | 652.0 | |
| 0.00 | 2.58 | 0.00 | 1.67 | -23.58 | 79.30 | 26.32 | 219.10 | 0.6467 | 689.0 | 611.0 | |
| 0.00 | 0.98 | 0.00 | 0.62 | -22.31 | 79.03 | 26.06 | 220.19 | 0.6320 | 765.0 | 580.5 | |
| 0.00 | 1.87 | 0.00 | 1.17 | -22.55 | 76.60 | 23.62 | 217.24 | 0.6137 | 457.0 | 373.9 | |
| 0.00 | 1.87 | 0.00 | 1.12 | -19.63 | 75.03 | 22.06 | 218.60 | 0.5691 | 693.0 | 508.4 | |
| 0.00 | 2.58 | 0.00 | 1.59 | -22.28 | 74.78 | 21.80 | 215.37 | 0.5959 | 568.0 | 486.0 | |
| 0.00 | 0.89 | 0.00 | 0.54 | -23.24 | 70.78 | 17.81 | 209.27 | 0.5769 | -614.0 | -448.7 | |
| 0.00 | 1.16 | 0.00 | 0.71 | -24.92 | 70.50 | 17.52 | 207.41 | 0.5955 | -712.0 | -590.4 | |
| 0.00 | 1.51 | 0.00 | 0.92 | -24.21 | 69.50 | 16.52 | 206.66 | 0.5803 | -849.0 | -689.4 | |
| 0.00 | 1.16 | 0.00 | 0.71 | -24.93 | 68.97 | 16.00 | 205.34 | 0.5861 | -801.0 | -639.6 | |
| 0.44 | 6.58 | 0.27 | 4.01 | -24.98 | 68.42 | 15.45 | 204.55 | 0.5834 | -847.0 | -637.4 | |
| 0.00 | 0.80 | 0.00 | 0.48 | -25.23 | 64.24 | 11.26 | 198.30 | 0.5650 | -648.0 | -509.2 | |
| 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. | |