SDO HMI 2014-04-05 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.85 | 461.50 | 42.15 | 250.21 | 12.46 | 13.51 | -14.90 | 38.26 | 0.4074 | -700.5 | -335.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.58 | 0.00 | 0.87 | 15.02 | 15.18 | -13.24 | 31.50 | 0.4251 | 608.0 | 557.2 | |
| 74.51 | 417.35 | 40.33 | 226.07 | 12.53 | 13.83 | -14.58 | 37.56 | 0.4049 | -1438.5 | -440.1 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 5.08 | 13.69 | -14.73 | 52.55 | 0.3204 | 918.0 | 683.3 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 8.91 | 13.38 | -15.04 | 44.72 | 0.3659 | 856.0 | 663.2 | |
| 0.88 | -2.00 | 0.48 | -2.00 | 12.98 | 12.69 | -15.73 | 38.98 | 0.4217 | -614.5 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 11.78 | 12.54 | -15.88 | 41.14 | 0.4088 | -497.0 | -357.9 | |
| 2.02 | -2.00 | 1.10 | -2.00 | 12.36 | 12.41 | -16.01 | 40.45 | 0.4170 | -800.2 | 999999 | |
| 0.44 | 2.55 | 0.24 | 1.38 | 11.54 | 12.39 | -16.02 | 41.81 | 0.4074 | -666.6 | -454.8 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 11.76 | 12.25 | -16.16 | 41.69 | 0.4115 | -381.0 | -274.9 | |
| 0.00 | 3.08 | 0.00 | 1.68 | 12.53 | 12.08 | -16.34 | 40.76 | 0.4224 | -447.0 | -414.1 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 15.81 | 11.64 | -16.78 | 36.74 | 0.4662 | 636.0 | 603.4 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 9.70 | 12.02 | -16.40 | 45.71 | 0.3905 | 776.0 | 500.9 | |
| 0.00 | 1.67 | 0.00 | 0.91 | 11.03 | 11.63 | -16.79 | 44.01 | 0.4098 | 846.0 | 672.3 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 11.60 | 11.56 | -16.86 | 43.16 | 0.4170 | 120.0 | 179.7 | |
| 0.00 | 1.58 | 0.00 | 0.86 | 11.41 | 11.51 | -16.91 | 43.56 | 0.4154 | 717.0 | 582.2 | |
| 0.00 | 1.50 | 0.00 | 0.83 | 15.08 | 11.25 | -17.17 | 38.37 | 0.4611 | 702.0 | 547.6 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 11.63 | 10.72 | -17.69 | 44.50 | 0.4265 | 954.0 | 867.3 | |
| 0.00 | 10.91 | 0.00 | 5.99 | 12.29 | 10.68 | -17.74 | 43.48 | 0.4344 | 1140.0 | 776.5 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 11.95 | 10.57 | -17.84 | 44.21 | 0.4317 | 906.0 | 691.6 | |
| 0.00 | 2.29 | 0.00 | 1.26 | 12.52 | 10.47 | -17.95 | 43.44 | 0.4393 | 607.0 | 568.0 | |
| 0.00 | 0.62 | 0.00 | 0.34 | 11.20 | 10.33 | -18.08 | 45.85 | 0.4262 | 716.0 | 545.7 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 11.71 | 10.20 | -18.21 | 45.19 | 0.4332 | 748.0 | 562.0 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 11.39 | 10.16 | -18.26 | 45.79 | 0.4302 | 851.0 | 627.3 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 12.22 | 10.01 | -18.41 | 44.66 | 0.4410 | 624.0 | 458.3 | |
| 0.00 | 2.20 | 0.00 | 1.20 | 9.07 | 8.75 | -19.66 | 52.06 | 0.4231 | 767.0 | 674.1 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 11.79 | 8.12 | -20.30 | 48.16 | 0.4577 | 750.0 | 619.2 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 10.93 | 6.25 | -22.17 | 52.10 | 0.4714 | 680.0 | 551.9 | |
| 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. | |