SDO HMI 2013-03-30 09:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.48 | 253.36 | 26.52 | 138.58 | 14.94 | 255.18 | 12.77 | 329.63 | 0.4245 | -930.7 | -337.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.81 | 0.00 | 1.57 | 17.18 | 257.07 | 14.66 | 328.85 | 0.4692 | -682.0 | -578.3 | |
| 0.00 | 0.79 | 0.00 | 0.44 | 16.30 | 256.87 | 14.46 | 328.15 | 0.4560 | 353.0 | 329.2 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 17.34 | 256.89 | 14.48 | 329.34 | 0.4698 | -668.0 | -566.3 | |
| 0.00 | 1.84 | 0.00 | 0.97 | 7.66 | 255.46 | 13.05 | 317.43 | 0.3322 | -741.0 | -581.5 | |
| 26.30 | 225.84 | 14.40 | 123.62 | 14.90 | 255.65 | 13.24 | 328.69 | 0.4276 | -1190.9 | -322.1 | |
| 0.00 | 3.59 | 0.00 | 1.93 | 12.49 | 255.03 | 12.62 | 326.68 | 0.3901 | -736.0 | -884.6 | |
| 0.00 | 2.02 | 0.00 | 1.14 | 19.24 | 255.19 | 12.78 | 334.27 | 0.4831 | -809.0 | -659.1 | |
| 0.00 | 1.75 | 0.00 | 0.95 | 13.79 | 254.79 | 12.38 | 328.97 | 0.4056 | -990.0 | -830.0 | |
| 21.39 | -5.00 | 11.69 | -5.00 | 15.17 | 254.84 | 12.43 | 330.59 | 0.4248 | -1199.1 | 999999 | |
| 0.00 | 4.21 | 0.00 | 2.26 | 12.67 | 254.70 | 12.29 | 327.64 | 0.3896 | -986.0 | -904.5 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 14.44 | 253.69 | 11.28 | 332.06 | 0.4059 | -828.0 | -690.1 | |
| 0.00 | 1.58 | 0.00 | 0.86 | 14.76 | 253.58 | 11.17 | 332.66 | 0.4096 | -839.0 | -652.2 | |
| 0.00 | 1.40 | 0.00 | 0.75 | 12.30 | 252.24 | 9.83 | 332.65 | 0.3647 | -681.0 | -507.2 | |
| 0.79 | 3.59 | 0.43 | 1.94 | 14.91 | 251.64 | 9.22 | 337.03 | 0.3986 | 849.7 | 754.1 | |
| 0.00 | 1.93 | 0.00 | 1.04 | 14.67 | 250.81 | 8.40 | 338.67 | 0.3901 | 777.0 | 640.3 | |
| 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. | |