SDO HMI 2014-03-30 15:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.70 | 199.53 | 62.44 | 313.80 | -13.05 | 174.59 | 72.49 | 258.41 | 0.9496 | 440.6 | 82.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.87 | 51.88 | 17.73 | 85.74 | -11.99 | 175.33 | 73.24 | 259.49 | 0.9540 | 349.9 | -144.0 | |
| 3.86 | 14.55 | 5.92 | 22.37 | -11.56 | 174.21 | 72.11 | 260.00 | 0.9482 | 502.9 | 443.7 | |
| 2.89 | -2.00 | 4.46 | -2.00 | -11.98 | 174.28 | 72.19 | 259.56 | 0.9484 | 567.5 | 999999 | |
| 22.08 | 124.17 | 34.33 | 194.17 | -13.64 | 174.55 | 72.45 | 257.79 | 0.9494 | 578.5 | 152.2 | |
| 0.00 | 1.23 | 0.00 | 1.80 | -11.81 | 173.28 | 71.19 | 259.79 | 0.9429 | 345.0 | 430.4 | |
| 0.00 | 0.53 | 0.00 | 0.76 | -12.69 | 173.08 | 70.98 | 258.86 | 0.9415 | 513.0 | 454.0 | |
| 0.00 | 0.96 | 0.00 | 1.32 | -15.04 | 171.83 | 69.73 | 256.39 | 0.9337 | 414.0 | 360.3 | |
| 0.00 | 1.40 | 0.00 | 1.76 | -12.99 | 169.65 | 67.56 | 258.67 | 0.9202 | -259.0 | -152.7 | |
| 0.00 | 0.70 | 0.00 | 0.88 | -13.20 | 169.69 | 67.60 | 258.44 | 0.9204 | -296.0 | -218.8 | |
| 0.00 | 0.96 | 0.00 | 1.21 | -13.35 | 169.78 | 67.68 | 258.28 | 0.9209 | -285.0 | -266.3 | |
| 0.00 | 0.96 | 0.00 | 1.23 | -14.29 | 170.18 | 68.09 | 257.25 | 0.9235 | 327.0 | 287.7 | |
| 0.00 | 0.70 | 0.00 | 0.88 | -13.95 | 169.64 | 67.54 | 257.63 | 0.9199 | -92.0 | -90.1 | |
| 0.00 | 0.79 | 0.00 | 1.03 | -15.59 | 170.72 | 68.63 | 255.82 | 0.9268 | 140.0 | 117.9 | |
| 0.00 | 0.70 | 0.00 | 0.65 | -14.00 | 160.53 | 58.44 | 257.60 | 0.8486 | -461.0 | -409.5 | |
| 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. | |