SDO HMI 2014-03-07 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.94 | 274.19 | 66.88 | 287.77 | -13.50 | 109.59 | 62.64 | 258.56 | 0.8813 | 358.7 | 224.4 | |
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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 |
| 0.00 | 1.64 | 0.00 | 2.25 | -15.16 | 116.87 | 69.92 | 256.50 | 0.9339 | 125.0 | 96.9 | |
| 11.25 | 32.37 | 15.28 | 43.73 | -15.64 | 116.69 | 69.74 | 255.99 | 0.9327 | 481.4 | 355.6 | |
| 0.00 | 0.52 | 0.00 | 0.63 | -11.24 | 113.48 | 66.53 | 260.89 | 0.9129 | 383.0 | 427.5 | |
| 4.76 | 7.27 | 5.51 | 8.41 | -11.48 | 112.45 | 65.50 | 260.68 | 0.9055 | 472.7 | 328.7 | |
| 0.00 | 1.30 | 0.00 | 1.67 | -16.87 | 115.43 | 68.48 | 254.69 | 0.9247 | 482.0 | 410.8 | |
| 0.87 | 2.94 | 1.07 | 3.64 | -15.93 | 114.41 | 67.46 | 255.73 | 0.9181 | -134.1 | -75.3 | |
| 0.00 | 0.95 | 0.00 | 1.18 | -17.13 | 114.53 | 67.58 | 254.43 | 0.9188 | -96.0 | -50.5 | |
| 0.00 | 0.78 | 0.00 | 0.87 | -12.67 | 111.61 | 64.66 | 259.40 | 0.8990 | -291.0 | -223.3 | |
| 0.00 | 0.52 | 0.00 | 0.63 | -17.31 | 113.77 | 66.82 | 254.24 | 0.9137 | 133.0 | 159.0 | |
| 9.87 | 22.24 | 11.61 | 26.15 | -18.26 | 113.05 | 66.10 | 253.19 | 0.9088 | -378.0 | -217.6 | |
| 0.00 | 1.04 | 0.00 | 1.14 | -15.49 | 110.95 | 63.99 | 256.26 | 0.8935 | -511.0 | -369.5 | |
| 4.85 | 14.28 | 4.95 | 14.57 | -12.81 | 108.74 | 61.78 | 259.34 | 0.8763 | -386.0 | -72.1 | |
| 29.34 | 186.78 | 28.46 | 181.38 | -12.29 | 107.01 | 60.06 | 259.97 | 0.8619 | 882.6 | 278.2 | |
| 0.00 | 0.35 | 0.00 | 0.34 | -14.56 | 107.21 | 60.26 | 257.34 | 0.8634 | -105.0 | -49.2 | |
| 0.00 | 0.43 | 0.00 | 0.42 | -15.50 | 107.28 | 60.32 | 256.25 | 0.8640 | -567.0 | -467.0 | |
| 0.00 | 0.78 | 0.00 | 0.76 | -14.97 | 107.03 | 60.08 | 256.85 | 0.8619 | -610.0 | -501.9 | |
| 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. | |