SDO HMI 2014-11-10 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.06 | 156.07 | 37.27 | 231.69 | -11.16 | 305.06 | -69.33 | 103.12 | 0.9436 | -341.7 | -278.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.43 | 0.00 | 0.40 | -11.19 | 318.55 | -55.84 | 105.59 | 0.8449 | 474.0 | 500.6 | |
| 0.00 | 0.95 | 0.00 | 0.87 | -11.04 | 318.54 | -55.85 | 105.41 | 0.8447 | 139.0 | 176.6 | |
| 1.03 | 2.33 | 1.17 | 2.64 | -11.73 | 311.73 | -62.67 | 104.79 | 0.9015 | 419.2 | 344.4 | |
| 0.00 | 0.78 | 0.00 | 0.92 | -11.34 | 310.46 | -63.94 | 104.14 | 0.9101 | 277.0 | 215.7 | |
| 0.00 | 3.62 | 0.00 | 4.66 | -12.67 | 308.54 | -65.85 | 105.25 | 0.9244 | 472.0 | 249.5 | |
| 0.00 | 0.69 | 0.00 | 0.92 | -11.25 | 307.55 | -66.84 | 103.58 | 0.9293 | 415.0 | 358.2 | |
| 0.00 | 0.95 | 0.00 | 1.27 | -11.60 | 307.39 | -67.01 | 103.92 | 0.9307 | 160.0 | 116.1 | |
| 0.00 | 0.95 | 0.00 | 1.42 | -14.46 | 305.30 | -69.09 | 106.61 | 0.9454 | -480.0 | -463.3 | |
| 0.86 | 4.40 | 1.14 | 5.79 | -10.31 | 307.43 | -66.96 | 102.56 | 0.9292 | 38.6 | 323.3 | |
| 0.00 | 1.38 | 0.00 | 1.90 | -11.57 | 306.76 | -67.63 | 103.80 | 0.9344 | 75.0 | 39.2 | |
| 0.00 | 3.79 | 0.00 | 5.77 | -14.20 | 304.95 | -69.44 | 106.28 | 0.9471 | -591.0 | -495.2 | |
| 0.00 | 3.10 | 0.00 | 4.32 | -11.31 | 306.49 | -67.91 | 103.48 | 0.9359 | -469.0 | -411.1 | |
| 0.00 | 0.95 | 0.00 | 1.35 | -11.95 | 305.99 | -68.41 | 104.08 | 0.9394 | -422.0 | -396.6 | |
| 0.00 | 7.33 | 0.00 | 10.80 | -12.66 | 305.41 | -68.98 | 104.74 | 0.9432 | -490.0 | -477.1 | |
| 0.00 | 1.47 | 0.00 | 2.27 | -14.00 | 304.55 | -69.84 | 106.02 | 0.9491 | -386.0 | -308.8 | |
| 4.22 | 20.78 | 5.88 | 28.74 | -10.65 | 306.41 | -67.99 | 102.76 | 0.9358 | -597.2 | -513.7 | |
| 0.00 | 1.12 | 0.00 | 1.61 | -10.96 | 305.76 | -68.64 | 103.00 | 0.9399 | -365.0 | -393.9 | |
| 0.00 | 0.95 | 0.00 | 1.37 | -11.21 | 305.54 | -68.85 | 103.24 | 0.9413 | -527.0 | -490.1 | |
| 1.03 | 2.67 | 1.50 | 3.87 | -10.73 | 305.53 | -68.86 | 102.72 | 0.9410 | -645.2 | -593.5 | |
| 3.53 | 18.97 | 5.29 | 28.57 | -11.28 | 304.90 | -69.49 | 103.22 | 0.9450 | -582.3 | -504.8 | |
| 0.00 | 2.50 | 0.00 | 4.13 | -13.86 | 303.26 | -71.14 | 105.68 | 0.9556 | -488.0 | -377.2 | |
| 0.00 | 0.78 | 0.00 | 1.16 | -10.73 | 304.84 | -69.55 | 102.64 | 0.9449 | -540.0 | -530.1 | |
| 0.00 | 3.88 | 0.00 | 6.64 | -13.99 | 302.67 | -71.72 | 105.73 | 0.9585 | 164.0 | 148.3 | |
| 0.00 | 1.90 | 0.00 | 3.04 | -12.42 | 303.68 | -70.71 | 104.24 | 0.9524 | -431.0 | -371.4 | |
| 0.00 | 0.95 | 0.00 | 1.54 | -12.56 | 303.40 | -70.99 | 104.35 | 0.9539 | -325.0 | -323.7 | |
| 0.00 | 0.78 | 0.00 | 1.31 | -13.43 | 302.80 | -71.59 | 105.16 | 0.9575 | -313.0 | -260.1 | |
| 4.31 | 26.73 | 6.50 | 41.22 | -10.38 | 304.58 | -69.81 | 102.23 | 0.9461 | -624.6 | -392.5 | |
| 0.00 | 1.55 | 0.00 | 2.51 | -12.31 | 303.47 | -70.92 | 104.10 | 0.9534 | -437.0 | -396.0 | |
| 0.60 | 1.98 | 1.02 | 3.35 | -13.15 | 302.81 | -71.59 | 104.87 | 0.9573 | -256.3 | -258.1 | |
| 0.00 | 2.24 | 0.00 | 3.88 | -13.66 | 302.42 | -71.97 | 105.35 | 0.9595 | 408.0 | 332.7 | |
| 0.00 | 0.26 | 0.00 | 0.42 | -12.30 | 303.20 | -71.20 | 104.04 | 0.9548 | -106.0 | -112.0 | |
| 0.00 | 33.19 | 0.00 | 50.27 | -9.81 | 304.51 | -69.89 | 101.62 | 0.9461 | 0.0 | -178.0 | |
| 2.50 | -27.00 | 3.84 | -27.00 | -10.22 | 304.21 | -70.18 | 102.01 | 0.9480 | -424.8 | 999999 | |
| 6.98 | -27.00 | 10.93 | -27.00 | -10.67 | 303.89 | -70.51 | 102.44 | 0.9500 | -429.0 | 999999 | |
| 0.00 | 1.72 | 0.00 | 2.76 | -10.45 | 303.45 | -70.94 | 102.15 | 0.9522 | -166.0 | -114.8 | |
| 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. | |