SDO HMI 2014-04-07 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.99 | 401.26 | 41.35 | 221.34 | 12.81 | 13.39 | 17.95 | 316.79 | 0.4408 | -1137.0 | -393.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.48 | 11.06 | 14.28 | 18.84 | 312.50 | 0.4316 | -784.0 | -694.9 | |
| 43.04 | 370.01 | 23.73 | 204.11 | 12.56 | 13.67 | 18.23 | 315.93 | 0.4409 | -1566.0 | -435.3 | |
| 1.67 | -2.00 | 0.92 | -2.00 | 13.18 | 13.43 | 17.99 | 317.31 | 0.4453 | -836.6 | 999999 | |
| 27.02 | -2.00 | 14.90 | -2.00 | 12.98 | 13.19 | 17.75 | 317.38 | 0.4405 | -1265.9 | 999999 | |
| 0.00 | 1.94 | 0.00 | 1.05 | 10.58 | 12.99 | 17.55 | 313.67 | 0.4116 | 940.0 | 729.8 | |
| 0.00 | 3.87 | 0.00 | 2.16 | 14.68 | 13.26 | 17.82 | 319.82 | 0.4608 | 868.0 | 579.9 | |
| 2.29 | 8.19 | 1.27 | 4.55 | 14.19 | 13.19 | 17.75 | 319.23 | 0.4544 | -804.6 | -354.8 | |
| 0.00 | 4.14 | 0.00 | 2.30 | 14.88 | 12.53 | 17.09 | 321.28 | 0.4559 | 716.0 | 688.9 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 12.57 | 12.16 | 16.72 | 318.43 | 0.4249 | -738.0 | -668.9 | |
| 0.00 | 1.23 | 0.00 | 0.68 | 15.01 | 11.63 | 16.19 | 322.96 | 0.4490 | -488.0 | -405.8 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 14.48 | 11.20 | 15.76 | 322.96 | 0.4385 | -846.0 | -656.2 | |
| 0.97 | 4.40 | 0.53 | 2.43 | 14.71 | 11.16 | 15.72 | 323.36 | 0.4408 | -934.1 | -701.0 | |
| 0.00 | 2.46 | 0.00 | 1.33 | 11.95 | 10.40 | 14.96 | 320.58 | 0.3993 | 725.0 | 482.0 | |
| 0.00 | 2.02 | 0.00 | 1.09 | 11.40 | 9.73 | 14.29 | 320.94 | 0.3857 | 670.0 | 416.1 | |
| 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. | |