SDO HMI 2014-09-04 04:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.60 | 0.00 | 11.30 | 8.58 | 182.39 | 3.42 | 197.43 | 0.1260 | -323.5 | -236.6 | |
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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 | 1.07 | 0.00 | 0.54 | 4.36 | 187.81 | 8.84 | 252.33 | 0.1615 | -714.0 | -540.5 | |
| 0.00 | 1.79 | 0.00 | 0.90 | 6.08 | 187.80 | 8.83 | 263.01 | 0.1546 | -927.0 | -767.1 | |
| 0.00 | 1.88 | 0.00 | 0.94 | 6.18 | 187.44 | 8.47 | 263.32 | 0.1481 | -898.0 | -677.5 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 5.97 | 187.28 | 8.31 | 261.75 | 0.1459 | -715.0 | -506.8 | |
| 0.00 | 2.50 | 0.00 | 1.25 | 11.32 | 185.97 | 7.00 | 301.07 | 0.1402 | -987.0 | -796.5 | |
| 0.00 | 2.32 | 0.00 | 1.16 | 10.86 | 185.96 | 6.99 | 298.21 | 0.1363 | -969.0 | -827.4 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 11.20 | 185.54 | 6.57 | 301.94 | 0.1328 | -853.0 | -677.7 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 5.94 | 185.38 | 6.41 | 258.87 | 0.1137 | -943.0 | -756.7 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 6.07 | 185.10 | 6.14 | 259.48 | 0.1086 | -858.0 | -617.8 | |
| 0.00 | 2.68 | 0.00 | 1.33 | 10.17 | 178.87 | -0.10 | 2.01 | 0.0514 | 991.0 | 717.3 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 8.44 | 176.48 | -2.49 | 63.88 | 0.0481 | 938.0 | 785.3 | |
| 0.00 | 2.59 | 0.00 | 1.30 | 11.26 | 171.14 | -7.83 | 61.92 | 0.1522 | 870.0 | 587.2 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 8.25 | 170.43 | -8.54 | 82.60 | 0.1488 | 860.0 | 686.8 | |
| 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. | |