SDO HMI 2014-03-06 00:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.07 | 118.18 | 36.77 | 145.15 | -9.96 | 359.67 | -67.02 | 97.72 | 0.9166 | 473.6 | 209.3 | |
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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 | 0.61 | -15.89 | 0.67 | -66.03 | 104.19 | 0.9083 | 319.0 | 318.5 | |
| 10.72 | 98.99 | 13.00 | 119.74 | -10.45 | 360.00 | -66.70 | 98.23 | 0.9143 | 698.0 | 308.9 | |
| 14.26 | -2.00 | 17.21 | -2.00 | -9.55 | 0.14 | -66.56 | 97.25 | 0.9138 | 639.3 | 999999 | |
| 1.64 | -2.00 | 2.00 | -2.00 | -10.10 | 359.91 | -66.78 | 97.86 | 0.9151 | 529.8 | 999999 | |
| 0.95 | 4.50 | 1.16 | 5.47 | -8.17 | 359.95 | -66.74 | 95.75 | 0.9157 | -330.7 | -438.7 | |
| 0.00 | 1.64 | 0.00 | 2.04 | -9.55 | 359.36 | -67.34 | 97.30 | 0.9191 | -333.0 | -305.6 | |
| 0.00 | 0.52 | 0.00 | 0.67 | -10.38 | 358.18 | -68.52 | 98.28 | 0.9266 | 375.0 | 282.2 | |
| 1.64 | 3.54 | 2.16 | 4.67 | -10.75 | 357.92 | -68.78 | 98.69 | 0.9281 | 219.4 | 110.9 | |
| 0.00 | 3.89 | 0.00 | 5.36 | -10.23 | 356.87 | -69.82 | 98.21 | 0.9348 | -454.0 | -381.9 | |
| 0.00 | 1.21 | 0.00 | 1.63 | -8.88 | 357.49 | -69.20 | 96.72 | 0.9316 | 428.0 | 354.5 | |
| 0.00 | 0.78 | 0.00 | 1.08 | -9.97 | 356.73 | -69.96 | 97.94 | 0.9358 | -12.0 | -54.1 | |
| 0.00 | 0.86 | 0.00 | 1.40 | -14.14 | 353.31 | -73.38 | 102.57 | 0.9534 | -402.0 | -388.7 | |
| 0.86 | 1.73 | 1.24 | 2.48 | -9.62 | 356.09 | -70.61 | 97.62 | 0.9398 | -335.4 | -345.4 | |
| 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. | |