SDO HMI 2014-10-14 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 |
| 70.77 | 461.84 | 40.46 | 264.25 | -21.04 | 17.19 | 13.31 | 205.50 | 0.5016 | 954.8 | 373.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.74 | -18.00 | 20.10 | 16.22 | 213.50 | 0.4833 | 909.0 | 775.7 | |
| 0.00 | 0.87 | 0.00 | 0.51 | -20.87 | 19.83 | 15.95 | 209.88 | 0.5174 | -550.0 | -512.8 | |
| 29.53 | 441.40 | 16.93 | 252.57 | -21.10 | 17.66 | 13.78 | 206.21 | 0.5053 | 1261.4 | 387.7 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -18.93 | 17.15 | 13.27 | 207.47 | 0.4725 | 1006.0 | 841.6 | |
| 38.62 | -3.00 | 22.05 | -3.00 | -20.95 | 17.06 | 13.18 | 205.35 | 0.4993 | 1414.8 | 999999 | |
| 0.00 | 1.75 | 0.00 | 1.01 | -22.12 | 16.73 | 12.85 | 203.78 | 0.5131 | -58.0 | -83.8 | |
| 1.83 | -3.00 | 1.04 | -3.00 | -20.87 | 16.59 | 12.71 | 204.64 | 0.4952 | 1169.4 | 999999 | |
| 0.00 | 2.45 | 0.00 | 1.45 | -25.25 | 16.40 | 12.52 | 200.84 | 0.5534 | 683.0 | 529.8 | |
| 0.00 | 1.75 | 0.00 | 0.99 | -21.57 | 14.81 | 10.93 | 200.99 | 0.4944 | 749.0 | 634.0 | |
| 0.00 | 0.61 | 0.00 | 0.34 | -18.60 | 14.57 | 10.69 | 203.05 | 0.4510 | -687.0 | -582.0 | |
| 0.00 | 1.22 | 0.00 | 0.68 | -18.73 | 14.49 | 10.61 | 202.77 | 0.4523 | -588.0 | -585.6 | |
| 0.00 | 3.06 | 0.00 | 1.73 | -20.89 | 14.40 | 10.52 | 200.79 | 0.4826 | 841.0 | 757.5 | |
| 0.00 | 1.22 | 0.00 | 0.70 | -21.96 | 13.89 | 10.01 | 199.08 | 0.4951 | -659.0 | -644.2 | |
| 0.00 | 0.87 | 0.00 | 0.50 | -21.75 | 13.84 | 9.96 | 199.15 | 0.4920 | -768.0 | -589.1 | |
| 0.79 | 2.36 | 0.44 | 1.33 | -21.04 | 13.47 | 9.59 | 198.99 | 0.4798 | -908.6 | -728.6 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -21.83 | 7.52 | 3.64 | 187.22 | 0.4710 | -610.0 | -455.0 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -28.50 | 4.89 | 1.01 | 181.57 | 0.5675 | -729.0 | -637.5 | |
| 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. | |