SDO HMI 2011-10-17 20:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.32 | 22.40 | 4.92 | 20.16 | 24.08 | 332.14 | -55.84 | 64.83 | 0.8352 | -362.1 | -339.7 | |
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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 | 1.31 | 0.00 | 1.03 | 20.64 | 337.40 | -50.58 | 68.02 | 0.7818 | -652.0 | -504.1 | |
| 0.00 | 0.78 | 0.00 | 0.66 | 24.13 | 334.83 | -53.15 | 64.24 | 0.8131 | -543.0 | -492.4 | |
| 0.00 | 0.61 | 0.00 | 0.53 | 24.39 | 334.00 | -53.98 | 64.10 | 0.8211 | -598.0 | -541.0 | |
| 1.74 | 9.42 | 1.50 | 8.13 | 23.39 | 333.94 | -54.04 | 65.32 | 0.8198 | -870.5 | -580.5 | |
| 0.00 | 0.70 | 0.00 | 0.60 | 23.04 | 333.98 | -54.00 | 65.73 | 0.8189 | -605.0 | -549.6 | |
| 2.01 | -4.00 | 1.74 | -4.00 | 23.49 | 333.66 | -54.33 | 65.25 | 0.8226 | -368.0 | 999999 | |
| 0.00 | 1.13 | 0.00 | 0.97 | 22.81 | 333.90 | -54.09 | 66.02 | 0.8193 | -588.0 | -598.1 | |
| 0.00 | 1.40 | 0.00 | 1.21 | 23.19 | 333.50 | -54.48 | 65.63 | 0.8235 | -386.0 | -311.6 | |
| 0.00 | 0.87 | 0.00 | 0.76 | 22.80 | 333.34 | -54.64 | 66.14 | 0.8243 | -501.0 | -415.6 | |
| 0.00 | 1.13 | 0.00 | 0.99 | 22.85 | 333.15 | -54.84 | 66.11 | 0.8261 | -246.0 | -218.7 | |
| 0.00 | 0.78 | 0.00 | 0.69 | 23.19 | 332.65 | -55.33 | 65.79 | 0.8311 | -344.0 | -233.6 | |
| 0.00 | 2.18 | 0.00 | 2.35 | 27.54 | 325.89 | -62.09 | 61.87 | 0.8904 | 327.0 | 245.3 | |
| 1.57 | 2.09 | 1.68 | 2.24 | 26.77 | 326.07 | -61.91 | 62.71 | 0.8883 | 404.1 | 347.8 | |
| 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. | |