SDO HMI 2014-08-14 18:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.33 | 77.30 | 27.13 | 90.42 | 16.05 | 22.99 | -65.75 | 75.33 | 0.9069 | -33.0 | 100.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.62 | 6.13 | 1.70 | 6.43 | 16.44 | 26.16 | -62.58 | 74.87 | 0.8839 | -620.4 | -564.5 | |
| 2.97 | 18.29 | 3.16 | 19.61 | 16.74 | 25.77 | -62.97 | 74.53 | 0.8870 | -609.1 | -312.6 | |
| 3.06 | -2.00 | 3.28 | -2.00 | 16.38 | 25.57 | -63.18 | 74.95 | 0.8885 | -526.4 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.88 | 15.97 | 25.30 | -63.44 | 75.41 | 0.8905 | -216.0 | -186.1 | |
| 0.00 | 1.26 | 0.00 | 1.38 | 16.13 | 25.00 | -63.75 | 75.23 | 0.8928 | -32.0 | 67.9 | |
| 0.00 | 0.90 | 0.00 | 1.00 | 17.07 | 24.34 | -64.40 | 74.19 | 0.8978 | -251.0 | -186.1 | |
| 5.32 | 10.09 | 6.08 | 11.55 | 16.65 | 23.64 | -65.11 | 74.67 | 0.9029 | -373.4 | -98.8 | |
| 0.00 | 1.71 | 0.00 | 2.03 | 16.79 | 22.53 | -66.21 | 74.53 | 0.9107 | 264.0 | 231.9 | |
| 0.00 | 2.25 | 0.00 | 2.66 | 15.21 | 22.70 | -66.05 | 76.27 | 0.9096 | 567.0 | 479.1 | |
| 8.11 | 24.42 | 9.95 | 29.88 | 15.39 | 21.70 | -67.04 | 76.07 | 0.9164 | 407.1 | 405.7 | |
| 1.35 | 3.42 | 1.77 | 4.47 | 16.45 | 20.11 | -68.63 | 74.90 | 0.9267 | 425.1 | 422.7 | |
| 0.00 | 1.35 | 0.00 | 1.76 | 16.07 | 20.13 | -68.62 | 75.31 | 0.9266 | 502.0 | 439.1 | |
| 0.00 | 1.08 | 0.00 | 1.44 | 16.33 | 19.58 | -69.17 | 75.02 | 0.9300 | 40.0 | 37.1 | |
| 0.90 | 5.59 | 1.19 | 7.33 | 15.72 | 19.77 | -68.97 | 75.68 | 0.9289 | 143.7 | 347.3 | |
| 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. | |