SDO HMI 2013-03-30 15:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.47 | 230.18 | 25.27 | 127.89 | 14.98 | 255.26 | 16.15 | 323.53 | 0.4539 | -1080.2 | -381.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.93 | 0.00 | 1.12 | 18.86 | 257.91 | 18.80 | 324.29 | 0.5245 | -754.0 | -434.7 | |
| 0.00 | 1.49 | 0.00 | 0.85 | 17.18 | 257.00 | 17.88 | 323.61 | 0.4965 | -804.0 | -728.3 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 17.50 | 256.74 | 17.62 | 324.40 | 0.4980 | -469.0 | -451.0 | |
| 22.69 | 210.29 | 12.63 | 116.89 | 14.93 | 255.65 | 16.54 | 322.81 | 0.4569 | -1185.3 | -343.1 | |
| 0.61 | -4.00 | 0.34 | -4.00 | 15.19 | 255.67 | 16.56 | 323.13 | 0.4603 | -722.9 | 999999 | |
| 0.00 | 5.43 | 0.00 | 2.97 | 12.84 | 255.24 | 16.12 | 320.50 | 0.4275 | -714.0 | -693.4 | |
| 1.93 | -4.00 | 1.07 | -4.00 | 14.88 | 255.16 | 16.05 | 323.57 | 0.4518 | -1105.3 | 999999 | |
| 0.00 | 7.45 | 0.00 | 4.06 | 12.61 | 254.87 | 15.76 | 320.79 | 0.4210 | -1092.0 | -763.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 14.65 | 255.02 | 15.90 | 323.51 | 0.4476 | -985.0 | -879.4 | |
| 0.53 | -4.00 | 0.29 | -4.00 | 14.78 | 254.77 | 15.65 | 324.10 | 0.4468 | -1156.8 | 999999 | |
| 19.71 | -4.00 | 10.94 | -4.00 | 15.23 | 254.77 | 15.66 | 324.70 | 0.4525 | -1199.9 | 999999 | |
| 0.00 | 1.40 | 0.00 | 0.77 | 13.59 | 254.59 | 15.47 | 322.76 | 0.4303 | -853.0 | -790.4 | |
| 0.00 | 0.61 | 0.00 | 0.35 | 17.95 | 254.55 | 15.43 | 328.41 | 0.4853 | -686.0 | -626.3 | |
| 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. | |