SDO HMI 2014-03-07 21:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.64 | 40.65 | 1.82 | 20.44 | -16.36 | 45.47 | 3.48 | 199.80 | 0.1729 | 315.9 | 273.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.42 | 0.00 | 1.22 | -15.67 | 48.10 | 6.11 | 214.86 | 0.1801 | 1096.0 | 861.2 | |
| 0.00 | 1.64 | 0.00 | 0.83 | -16.76 | 48.11 | 6.11 | 211.58 | 0.1955 | 878.0 | 560.2 | |
| 0.00 | 1.64 | 0.00 | 0.83 | -16.58 | 47.98 | 5.98 | 211.54 | 0.1918 | 878.0 | 801.6 | |
| 0.95 | 2.16 | 0.48 | 1.09 | -16.04 | 47.84 | 5.84 | 212.53 | 0.1827 | 1100.2 | 894.4 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -16.10 | 47.50 | 5.50 | 210.82 | 0.1806 | 796.0 | 652.5 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -16.35 | 47.07 | 5.07 | 208.15 | 0.1806 | 722.0 | 570.1 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -15.93 | 46.53 | 4.53 | 206.68 | 0.1700 | 871.0 | 687.1 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -16.71 | 46.55 | 4.55 | 204.76 | 0.1822 | 920.0 | 691.3 | |
| 0.61 | 10.03 | 0.30 | 5.04 | -15.81 | 46.28 | 4.28 | 205.72 | 0.1663 | 1186.7 | 863.4 | |
| 0.00 | 2.16 | 0.00 | 1.09 | -17.74 | 46.16 | 4.17 | 200.79 | 0.1960 | 1005.0 | 826.6 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -15.52 | 45.62 | 3.63 | 202.95 | 0.1571 | 1009.0 | 692.1 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -16.94 | 43.16 | 1.16 | 186.58 | 0.1702 | -547.0 | -583.2 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -15.80 | 43.12 | 1.13 | 187.26 | 0.1505 | -1013.0 | -907.0 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -17.09 | 43.07 | 1.07 | 185.97 | 0.1726 | -1082.0 | -872.9 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -16.40 | 42.88 | 0.88 | 185.31 | 0.1604 | -929.0 | -583.3 | |
| 2.08 | 6.75 | 1.04 | 3.39 | -16.88 | 42.75 | 0.76 | 184.33 | 0.1685 | -1095.1 | -954.7 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -16.64 | 42.38 | 0.39 | 182.27 | 0.1640 | -1006.0 | -758.3 | |
| 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. | |