SDO HMI 2014-05-15 21:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.81 | 160.27 | 23.75 | 105.81 | 15.20 | 248.88 | 37.73 | 296.67 | 0.6631 | -392.3 | -233.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.31 | 145.79 | 12.18 | 96.71 | 15.35 | 249.38 | 38.23 | 296.60 | 0.6697 | -728.7 | -317.4 | |
| 2.60 | -1.00 | 1.73 | -1.00 | 15.60 | 249.15 | 38.00 | 297.07 | 0.6683 | -808.8 | 999999 | |
| 11.58 | -1.00 | 7.65 | -1.00 | 15.27 | 248.92 | 37.77 | 296.75 | 0.6640 | -976.6 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.95 | 15.88 | 249.02 | 37.87 | 297.54 | 0.6681 | -532.0 | -412.7 | |
| 3.32 | -1.00 | 2.19 | -1.00 | 15.65 | 248.73 | 37.58 | 297.38 | 0.6636 | -872.3 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.68 | 11.92 | 247.32 | 36.17 | 292.75 | 0.6285 | 605.0 | 482.2 | |
| 0.00 | 1.97 | 0.00 | 1.25 | 11.81 | 246.77 | 35.62 | 292.89 | 0.6210 | 773.0 | 613.5 | |
| 0.00 | 1.44 | 0.00 | 0.90 | 11.62 | 246.59 | 35.44 | 292.69 | 0.6179 | 725.0 | 632.3 | |
| 0.00 | 1.62 | 0.00 | 1.02 | 13.84 | 246.30 | 35.15 | 296.20 | 0.6253 | 687.0 | 526.4 | |
| 0.00 | 1.80 | 0.00 | 1.14 | 14.34 | 246.12 | 34.97 | 297.05 | 0.6258 | 625.0 | 457.8 | |
| 0.00 | 1.08 | 0.00 | 0.68 | 13.71 | 245.97 | 34.82 | 296.20 | 0.6205 | 601.0 | 593.8 | |
| 0.00 | 0.45 | 0.00 | 0.28 | 14.39 | 245.71 | 34.56 | 297.38 | 0.6211 | 703.0 | 625.0 | |
| 0.00 | 1.53 | 0.00 | 0.95 | 12.90 | 245.27 | 34.12 | 295.41 | 0.6076 | 670.0 | 588.3 | |
| 0.00 | 0.72 | 0.00 | 0.44 | 14.25 | 242.29 | 31.14 | 299.49 | 0.5781 | 582.0 | 436.0 | |
| 0.00 | 1.35 | 0.00 | 0.81 | 13.76 | 241.93 | 30.78 | 299.01 | 0.5705 | 586.0 | 434.3 | |
| 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. | |