SDO HMI 2014-03-15 06:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.24 | 180.98 | 42.29 | 236.65 | 11.29 | 10.44 | 65.63 | 285.33 | 0.9274 | -116.6 | -96.0 | |
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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 | 0.52 | 0.00 | 0.72 | 10.77 | 11.83 | 67.02 | 284.46 | 0.9356 | -237.0 | -234.8 | |
| 6.95 | 107.27 | 9.85 | 147.72 | 11.76 | 12.07 | 67.26 | 285.45 | 0.9383 | -258.3 | -290.6 | |
| 7.65 | -2.00 | 10.51 | -2.00 | 11.56 | 11.42 | 66.61 | 285.38 | 0.9342 | -713.2 | 999999 | |
| 2.26 | -2.00 | 3.12 | -2.00 | 11.97 | 11.47 | 66.66 | 285.80 | 0.9350 | -474.3 | 999999 | |
| 1.48 | -2.00 | 1.94 | -2.00 | 11.59 | 10.38 | 65.57 | 285.66 | 0.9279 | -562.8 | 999999 | |
| 0.00 | 0.87 | 0.00 | 1.11 | 11.12 | 9.80 | 64.99 | 285.30 | 0.9235 | -433.0 | -410.2 | |
| 0.00 | 0.52 | 0.00 | 0.65 | 10.33 | 9.40 | 64.59 | 284.55 | 0.9198 | 6.0 | -24.7 | |
| 1.04 | 2.43 | 1.31 | 3.06 | 10.92 | 9.35 | 64.54 | 285.18 | 0.9203 | -55.1 | -152.2 | |
| 9.65 | 66.59 | 11.71 | 80.17 | 10.55 | 8.57 | 63.76 | 284.98 | 0.9145 | 413.3 | 260.0 | |
| 1.30 | -9.00 | 1.56 | -9.00 | 10.47 | 8.20 | 63.39 | 284.99 | 0.9119 | 850.6 | 999999 | |
| 1.91 | -9.00 | 2.29 | -9.00 | 10.85 | 8.20 | 63.40 | 285.38 | 0.9125 | 325.3 | 999999 | |
| 0.00 | 0.52 | 0.00 | 0.63 | 11.42 | 8.09 | 63.28 | 286.03 | 0.9127 | -206.0 | -147.2 | |
| 0.00 | 1.39 | 0.00 | 1.59 | 11.13 | 6.84 | 62.03 | 286.03 | 0.9035 | 581.0 | 460.0 | |
| 0.00 | 0.87 | 0.00 | 1.00 | 11.40 | 6.81 | 62.01 | 286.33 | 0.9038 | 433.0 | 346.9 | |
| 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. | |