SDO HMI 2014-07-06 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.36 | 37.16 | 3.33 | 19.41 | -14.09 | 254.68 | 5.07 | 195.63 | 0.3176 | 310.6 | 200.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 0.86 | -13.60 | 259.42 | 9.81 | 209.56 | 0.3372 | 920.0 | 756.4 | |
| 0.00 | 2.18 | 0.00 | 1.15 | -13.88 | 259.15 | 9.54 | 208.45 | 0.3391 | 636.0 | 602.1 | |
| 0.00 | 2.27 | 0.00 | 1.19 | -13.94 | 258.48 | 8.87 | 206.68 | 0.3348 | 720.0 | 618.8 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -14.22 | 258.40 | 8.79 | 206.07 | 0.3384 | 769.0 | 647.8 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -14.35 | 258.24 | 8.63 | 205.50 | 0.3392 | 683.0 | 486.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -11.13 | 256.38 | 6.77 | 204.74 | 0.2776 | 894.0 | 595.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -12.99 | 255.80 | 6.19 | 200.40 | 0.3026 | 796.0 | 607.2 | |
| 6.36 | 11.08 | 3.33 | 5.80 | -14.48 | 255.17 | 5.56 | 196.97 | 0.3228 | 1003.7 | 793.3 | |
| 0.00 | 1.82 | 0.00 | 0.95 | -14.64 | 254.10 | 4.49 | 193.73 | 0.3206 | 1055.0 | 852.0 | |
| 0.00 | 0.82 | 0.00 | 0.43 | -14.82 | 253.37 | 3.77 | 191.46 | 0.3210 | 554.0 | 467.9 | |
| 0.00 | 4.27 | 0.00 | 2.23 | -14.56 | 251.79 | 2.18 | 186.81 | 0.3125 | -1012.0 | -805.0 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -15.36 | 251.77 | 2.16 | 186.44 | 0.3257 | -845.0 | -723.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -14.98 | 251.67 | 2.06 | 186.28 | 0.3191 | -853.0 | -784.1 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -14.72 | 251.54 | 1.93 | 185.98 | 0.3147 | -997.0 | -828.1 | |
| 0.00 | 2.09 | 0.00 | 1.07 | -11.16 | 251.02 | 1.41 | 185.48 | 0.2543 | 876.0 | 729.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -14.98 | 250.95 | 1.34 | 184.08 | 0.3180 | -646.0 | -488.7 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -14.33 | 250.03 | 0.42 | 181.33 | 0.3066 | -888.0 | -636.4 | |
| 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. | |