SDO HMI 2014-06-05 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.76 | 286.20 | 25.24 | 142.31 | -4.47 | 301.65 | 1.72 | 202.73 | 0.0833 | 942.5 | 423.5 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.53 | 5.88 | 1.76 | 2.93 | -5.40 | 302.92 | 2.99 | 209.60 | 0.1056 | 1154.7 | 878.6 | |
| 0.00 | 3.35 | 0.00 | 1.67 | -5.36 | 302.58 | 2.65 | 206.89 | 0.1023 | 1211.0 | 955.3 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -5.67 | 302.03 | 2.10 | 200.79 | 0.1033 | 797.0 | 596.2 | |
| 38.27 | 237.96 | 19.02 | 118.25 | -4.14 | 301.91 | 1.98 | 206.31 | 0.0780 | 1486.3 | 464.7 | |
| 3.26 | 22.44 | 1.62 | 11.18 | -5.88 | 301.39 | 1.46 | 194.25 | 0.1035 | 1165.1 | 767.3 | |
| 1.36 | -4.00 | 0.67 | -4.00 | -4.02 | 301.39 | 1.46 | 200.63 | 0.0724 | 1087.9 | 999999 | |
| 2.44 | -5.00 | 1.22 | -5.00 | -6.04 | 301.15 | 1.22 | 191.64 | 0.1051 | 1091.0 | 999999 | |
| 1.90 | -5.00 | 0.95 | -5.00 | -5.88 | 300.84 | 0.91 | 189.00 | 0.1015 | 1184.3 | 999999 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -5.97 | 300.08 | 0.15 | 181.43 | 0.1019 | 714.0 | 541.0 | |
| 0.00 | 1.09 | 0.00 | 0.54 | -4.75 | 299.34 | -0.59 | 172.76 | 0.0812 | -1036.0 | -808.4 | |
| 0.00 | 2.44 | 0.00 | 1.22 | -7.38 | 298.20 | -1.73 | 166.64 | 0.1299 | -938.0 | -772.1 | |
| 0.00 | 4.07 | 0.00 | 2.04 | -8.57 | 297.52 | -2.41 | 164.15 | 0.1529 | -1074.0 | -834.2 | |
| 0.00 | 3.26 | 0.00 | 1.63 | -6.58 | 297.44 | -2.49 | 158.94 | 0.1205 | -912.0 | -817.5 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -6.58 | 296.95 | -2.98 | 155.25 | 0.1238 | -917.0 | -783.1 | |
| 0.00 | 1.27 | 0.00 | 0.63 | -4.32 | 295.22 | -4.71 | 131.60 | 0.1099 | -948.0 | -700.7 | |
| 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. | |