SDO HMI 2014-10-09 17:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.28 | 336.45 | 48.49 | 306.48 | -20.60 | 18.62 | -51.22 | 119.54 | 0.8410 | 728.7 | 182.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.98 | -19.66 | 20.84 | -49.01 | 119.47 | 0.8186 | 589.0 | 490.5 | |
| 0.00 | 1.49 | 0.00 | 1.30 | -20.41 | 20.51 | -49.33 | 120.17 | 0.8244 | 560.0 | 491.0 | |
| 2.37 | 324.62 | 2.08 | 295.85 | -20.54 | 20.11 | -49.73 | 120.13 | 0.8283 | 819.6 | 183.7 | |
| 1.58 | -3.00 | 1.41 | -3.00 | -20.60 | 19.48 | -50.36 | 119.91 | 0.8338 | 975.2 | 999999 | |
| 48.89 | -3.00 | 44.61 | -3.00 | -20.68 | 18.53 | -51.31 | 119.59 | 0.8420 | 862.3 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.61 | -17.62 | 19.50 | -50.34 | 116.58 | 0.8227 | 532.0 | 449.8 | |
| 0.00 | 0.88 | 0.00 | 0.76 | -17.76 | 19.39 | -50.45 | 116.69 | 0.8241 | 549.0 | 544.4 | |
| 0.00 | 1.23 | 0.00 | 1.21 | -23.35 | 16.42 | -53.42 | 121.60 | 0.8676 | 431.0 | 334.8 | |
| 0.00 | 1.14 | 0.00 | 0.99 | -17.61 | 19.15 | -50.69 | 116.43 | 0.8257 | 380.0 | 318.5 | |
| 0.00 | 0.79 | 0.00 | 0.70 | -17.86 | 18.55 | -51.29 | 116.46 | 0.8318 | 382.0 | 299.6 | |
| 0.00 | 0.96 | 0.00 | 0.87 | -18.15 | 17.87 | -51.97 | 116.51 | 0.8386 | 256.0 | 238.7 | |
| 0.44 | 1.75 | 0.39 | 1.56 | -16.91 | 18.02 | -51.82 | 115.17 | 0.8332 | -626.0 | -545.5 | |
| 0.00 | 0.96 | 0.00 | 0.90 | -17.47 | 16.44 | -53.40 | 115.20 | 0.8485 | -559.0 | -465.8 | |
| 0.00 | 0.79 | 0.00 | 0.75 | -14.39 | 14.45 | -55.39 | 111.05 | 0.8563 | -448.0 | -399.6 | |
| 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. | |