SDO HMI 2014-06-08 15:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.72 | 166.10 | 16.72 | 121.50 | -3.48 | 304.12 | 47.20 | 265.05 | 0.7373 | 458.9 | 242.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.72 | 151.33 | 16.72 | 111.44 | -3.44 | 304.49 | 47.56 | 265.15 | 0.7417 | 992.4 | 293.6 | |
| 0.00 | 1.09 | 0.00 | 0.77 | -2.85 | 302.71 | 45.79 | 265.81 | 0.7201 | 655.0 | 495.0 | |
| 0.00 | 1.18 | 0.00 | 0.83 | -3.46 | 302.05 | 45.13 | 264.91 | 0.7125 | -434.0 | -307.8 | |
| 0.00 | 0.91 | 0.00 | 0.64 | -4.46 | 301.82 | 44.89 | 263.47 | 0.7105 | 589.0 | 406.9 | |
| 0.00 | 1.27 | 0.00 | 0.88 | -2.54 | 301.36 | 44.43 | 266.15 | 0.7033 | 818.0 | 610.6 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -4.10 | 301.44 | 44.52 | 263.94 | 0.7056 | 375.0 | 515.7 | |
| 0.00 | 1.36 | 0.00 | 0.93 | -3.70 | 300.52 | 43.60 | 264.42 | 0.6938 | -621.0 | -539.7 | |
| 0.00 | 2.62 | 0.00 | 1.80 | -4.03 | 300.54 | 43.62 | 263.93 | 0.6943 | -493.0 | -369.4 | |
| 0.00 | 1.72 | 0.00 | 1.16 | -2.17 | 299.61 | 42.69 | 266.56 | 0.6811 | -768.0 | -616.4 | |
| 0.00 | 0.72 | 0.00 | 0.49 | -2.29 | 299.45 | 42.53 | 266.37 | 0.6791 | -715.0 | -621.2 | |
| 0.00 | 0.91 | 0.00 | 0.60 | -2.56 | 299.01 | 42.08 | 265.93 | 0.6735 | -562.0 | -470.1 | |
| 0.00 | 0.81 | 0.00 | 0.54 | -5.43 | 298.16 | 41.23 | 261.55 | 0.6657 | -633.0 | -532.3 | |
| 0.00 | 0.91 | 0.00 | 0.60 | -8.43 | 297.49 | 40.57 | 256.91 | 0.6628 | -528.0 | -506.7 | |
| 0.00 | 1.00 | 0.00 | 0.63 | -7.96 | 294.77 | 37.85 | 256.89 | 0.6262 | -636.0 | -554.8 | |
| 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. | |