SDO HMI 2014-03-30 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.09 | 227.45 | 56.55 | 325.67 | -13.13 | 174.36 | 70.62 | 258.40 | 0.9390 | 459.1 | 132.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.41 | 54.87 | 20.03 | 82.59 | -11.99 | 175.27 | 71.53 | 259.58 | 0.9448 | 467.4 | -82.4 | |
| 0.00 | 1.23 | 0.00 | 1.79 | -11.17 | 174.67 | 70.93 | 260.49 | 0.9416 | 359.0 | 318.5 | |
| 3.07 | 17.79 | 4.35 | 24.98 | -11.92 | 174.18 | 70.44 | 259.71 | 0.9385 | 524.5 | 460.9 | |
| 21.91 | 139.02 | 31.34 | 199.63 | -13.67 | 174.47 | 70.73 | 257.83 | 0.9398 | 660.7 | 178.3 | |
| 0.00 | 5.61 | 0.00 | 7.22 | -15.20 | 172.03 | 68.29 | 256.26 | 0.9246 | 656.0 | 449.9 | |
| 0.00 | 0.44 | 0.00 | 0.52 | -13.42 | 170.13 | 66.39 | 258.23 | 0.9121 | 24.0 | -69.6 | |
| 0.70 | 2.10 | 0.83 | 2.49 | -13.03 | 169.77 | 66.03 | 258.67 | 0.9097 | -358.8 | -229.1 | |
| 0.00 | 1.05 | 0.00 | 1.25 | -13.21 | 169.86 | 66.12 | 258.48 | 0.9103 | -192.0 | -208.3 | |
| 0.00 | 0.35 | 0.00 | 0.41 | -13.35 | 169.63 | 65.89 | 258.32 | 0.9086 | -435.0 | -436.0 | |
| 0.00 | 1.14 | 0.00 | 1.34 | -13.62 | 169.70 | 65.96 | 258.02 | 0.9091 | -259.0 | -246.0 | |
| 0.00 | 1.31 | 0.00 | 1.20 | -15.07 | 161.29 | 57.55 | 256.30 | 0.8408 | -338.0 | -326.8 | |
| 0.00 | 0.96 | 0.00 | 0.86 | -14.63 | 160.76 | 57.02 | 256.81 | 0.8358 | -334.0 | -254.4 | |
| 0.00 | 0.70 | 0.00 | 0.62 | -15.09 | 160.15 | 56.41 | 256.24 | 0.8302 | -532.0 | -507.0 | |
| 0.00 | 0.88 | 0.00 | 0.77 | -14.35 | 159.86 | 56.12 | 257.12 | 0.8272 | -448.0 | -409.4 | |
| 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. | |