SDO HMI 2014-08-01 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.03 | 43.91 | 7.99 | 25.08 | -20.80 | 249.19 | -13.66 | 153.63 | 0.4984 | 630.7 | 456.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.80 | -17.15 | 251.42 | -11.43 | 153.99 | 0.4335 | -803.0 | -695.2 | |
| 0.00 | 2.17 | 0.00 | 1.20 | -18.25 | 251.12 | -11.73 | 154.54 | 0.4510 | 703.0 | 588.1 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -17.99 | 250.94 | -11.91 | 153.94 | 0.4485 | 801.0 | 680.4 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -17.52 | 250.98 | -11.88 | 153.51 | 0.4418 | 729.0 | 482.7 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -22.23 | 250.54 | -12.31 | 157.12 | 0.5097 | 554.0 | 490.4 | |
| 0.00 | 2.72 | 0.00 | 1.57 | -22.96 | 250.43 | -12.42 | 157.54 | 0.5202 | 570.0 | 461.4 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -22.68 | 248.97 | -13.88 | 154.97 | 0.5253 | 776.0 | 590.7 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -22.86 | 248.88 | -13.97 | 154.99 | 0.5281 | 717.0 | 579.0 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -23.00 | 248.80 | -14.05 | 154.98 | 0.5305 | 346.0 | 391.2 | |
| 14.03 | 26.88 | 7.99 | 15.31 | -20.49 | 249.02 | -13.83 | 153.03 | 0.4957 | 947.4 | 595.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -22.90 | 248.68 | -14.18 | 154.70 | 0.5300 | 730.0 | 605.5 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -20.43 | 248.46 | -14.40 | 152.04 | 0.4990 | 522.0 | 436.5 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -19.21 | 247.50 | -15.35 | 149.20 | 0.4901 | 667.0 | 541.2 | |
| 0.00 | 1.00 | 0.00 | 0.65 | -29.65 | 242.72 | -20.13 | 152.50 | 0.6501 | -642.0 | -562.6 | |
| 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. | |