SDO HMI 2014-03-05 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.03 | 61.52 | 12.26 | 34.07 | -17.10 | 44.76 | -25.24 | 114.21 | 0.4484 | -141.1 | 130.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 0.57 | -19.54 | 47.75 | -22.25 | 121.87 | 0.4219 | -641.0 | -555.2 | |
| 1.30 | 20.74 | 0.71 | 11.30 | -16.89 | 46.94 | -23.06 | 115.29 | 0.4164 | 1181.2 | 797.4 | |
| 4.06 | -2.00 | 2.21 | -2.00 | -17.06 | 46.74 | -23.26 | 115.53 | 0.4201 | 922.3 | 999999 | |
| 0.52 | -2.00 | 0.28 | -2.00 | -16.75 | 46.68 | -23.32 | 114.79 | 0.4193 | 941.7 | 999999 | |
| 0.69 | 3.97 | 0.38 | 2.17 | -16.30 | 46.57 | -23.43 | 113.67 | 0.4184 | 1006.5 | 785.8 | |
| 0.69 | 2.16 | 0.38 | 1.18 | -16.51 | 45.97 | -24.03 | 113.71 | 0.4282 | 753.4 | 630.9 | |
| 1.64 | 3.80 | 0.91 | 2.10 | -17.43 | 45.02 | -24.98 | 115.02 | 0.4465 | 804.1 | 639.7 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -16.33 | 44.39 | -25.61 | 112.27 | 0.4502 | -769.0 | -696.8 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -16.22 | 43.99 | -26.01 | 111.79 | 0.4554 | -718.0 | -594.8 | |
| 7.43 | 22.99 | 4.18 | 12.92 | -17.50 | 43.06 | -26.94 | 113.86 | 0.4744 | -1080.3 | -781.5 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -16.21 | 43.16 | -26.84 | 111.27 | 0.4672 | -884.0 | -650.7 | |
| 5.70 | -10.00 | 3.21 | -10.00 | -17.33 | 42.78 | -27.22 | 113.35 | 0.4776 | -809.1 | 999999 | |
| 0.00 | 2.16 | 0.00 | 1.22 | -16.60 | 42.58 | -27.42 | 111.75 | 0.4771 | -774.0 | -639.5 | |
| 0.00 | 1.38 | 0.00 | 0.79 | -16.97 | 41.64 | -28.36 | 111.97 | 0.4919 | 657.0 | 394.7 | |
| 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. | |