| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 87.66 | 314.02 | 56.48 | 203.37 | -15.66 | 205.16 | -33.26 | 124.96 | 0.6457 | -36.2 | -188.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-30 16:00:37 UT
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 | 0.72 | 0.00 | 0.41 | -11.63 | 213.46 | -24.97 | 126.92 | 0.5192 | -488.0 | -375.4 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -14.53 | 209.01 | -29.41 | 126.67 | 0.5949 | 738.0 | 509.8 | |
| 2.78 | 4.39 | 1.77 | 2.80 | -18.07 | 208.15 | -30.27 | 130.55 | 0.6330 | 841.4 | 689.2 | |
| 0.00 | 0.98 | 0.00 | 0.61 | -14.75 | 208.62 | -29.81 | 126.61 | 0.6011 | 792.0 | 712.5 | |
| 0.00 | 1.70 | 0.00 | 1.06 | -14.92 | 208.52 | -29.91 | 126.76 | 0.6035 | 539.0 | 572.5 | |
| 0.90 | 2.24 | 0.57 | 1.43 | -17.99 | 207.91 | -30.51 | 130.23 | 0.6348 | 690.6 | 574.5 | |
| 1.16 | 3.13 | 0.75 | 2.01 | -18.20 | 207.76 | -30.67 | 130.35 | 0.6381 | 524.9 | 424.2 | |
| 0.00 | 1.34 | 0.00 | 0.87 | -18.88 | 207.51 | -30.92 | 130.98 | 0.6462 | 553.0 | 438.3 | |
| 0.00 | 1.07 | 0.00 | 0.66 | -13.98 | 208.08 | -30.34 | 125.06 | 0.6011 | 789.0 | 658.3 | |
| 30.26 | 122.40 | 18.88 | 76.71 | -14.83 | 207.91 | -30.51 | 126.09 | 0.6095 | 963.9 | 242.1 | |
| 4.66 | -10.00 | 2.92 | -10.00 | -15.29 | 207.80 | -30.62 | 126.62 | 0.6144 | 626.4 | 999999 | |
| 0.00 | 2.69 | 0.00 | 1.69 | -15.68 | 207.41 | -31.01 | 126.79 | 0.6217 | 355.0 | 407.8 | |
| 2.51 | -10.00 | 1.57 | -10.00 | -15.03 | 207.41 | -31.02 | 125.91 | 0.6167 | 469.4 | 999999 | |
| 1.16 | 2.60 | 0.75 | 1.66 | -16.55 | 206.66 | -31.76 | 127.28 | 0.6364 | 665.2 | 536.8 | |
| 0.00 | 1.97 | 0.00 | 1.29 | -18.61 | 206.17 | -32.25 | 129.47 | 0.6574 | 564.0 | 358.7 | |
| 4.75 | -10.00 | 3.01 | -10.00 | -15.34 | 206.66 | -31.77 | 125.68 | 0.6273 | -10.2 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -17.34 | 206.25 | -32.18 | 127.94 | 0.6468 | 559.0 | 471.1 | |
| 1.52 | -10.00 | 0.97 | -10.00 | -15.37 | 206.24 | -32.18 | 125.37 | 0.6321 | 501.9 | 999999 | |
| 0.00 | 1.52 | 0.00 | 0.97 | -15.14 | 205.76 | -32.66 | 124.67 | 0.6357 | -191.0 | -160.9 | |
| 0.00 | 3.31 | 0.00 | 2.11 | -14.18 | 205.48 | -32.94 | 123.16 | 0.6321 | 520.0 | 439.0 | |
| 0.54 | 1.43 | 0.35 | 0.93 | -15.48 | 205.06 | -33.36 | 124.57 | 0.6458 | -723.2 | -660.3 | |
| 0.00 | 1.70 | 0.00 | 1.10 | -15.32 | 205.02 | -33.41 | 124.32 | 0.6452 | -710.0 | -565.9 | |
| 0.00 | 1.61 | 0.00 | 1.04 | -15.03 | 204.96 | -33.47 | 123.89 | 0.6438 | -825.0 | -588.3 | |
| 0.00 | 2.51 | 0.00 | 1.64 | -16.11 | 204.57 | -33.86 | 124.99 | 0.6556 | -354.0 | -324.6 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -15.08 | 204.72 | -33.70 | 123.77 | 0.6468 | -709.0 | -654.0 | |
| 0.00 | 1.79 | 0.00 | 1.18 | -16.35 | 204.36 | -34.06 | 125.15 | 0.6595 | -705.0 | -694.8 | |
| 0.00 | 0.54 | 0.00 | 0.37 | -20.40 | 203.27 | -35.15 | 129.27 | 0.6994 | 181.0 | 221.0 | |
| 3.22 | 4.66 | 2.08 | 3.01 | -14.38 | 204.54 | -33.88 | 122.70 | 0.6439 | 552.7 | 393.2 | |
| 1.25 | 4.12 | 0.82 | 2.71 | -16.13 | 204.22 | -34.21 | 124.75 | 0.6595 | -903.7 | -711.5 | |
| 0.00 | 3.58 | 0.00 | 2.33 | -15.07 | 204.38 | -34.04 | 123.50 | 0.6504 | -557.0 | -579.5 | |
| 0.00 | 0.81 | 0.00 | 0.53 | -14.94 | 203.99 | -34.43 | 123.02 | 0.6539 | -555.0 | -485.7 | |
| 0.00 | 4.03 | 0.00 | 2.62 | -14.48 | 204.04 | -34.39 | 122.45 | 0.6503 | 514.0 | 382.2 | |
| 0.00 | 1.34 | 0.00 | 0.88 | -14.82 | 203.90 | -34.52 | 122.79 | 0.6540 | -718.0 | -623.3 | |
| 0.00 | 3.22 | 0.00 | 2.09 | -14.14 | 203.91 | -34.52 | 121.89 | 0.6494 | -774.0 | -508.2 | |
| 0.00 | 1.07 | 0.00 | 0.72 | -16.77 | 203.16 | -35.26 | 124.76 | 0.6751 | -563.0 | -544.2 | |
| 0.00 | 0.72 | 0.00 | 0.48 | -16.88 | 203.02 | -35.40 | 124.80 | 0.6774 | -586.0 | -541.9 | |
| 0.00 | 0.81 | 0.00 | 0.54 | -16.58 | 203.05 | -35.38 | 124.44 | 0.6751 | -415.0 | -393.8 | |
| 0.00 | 5.10 | 0.00 | 3.46 | -17.63 | 202.70 | -35.73 | 125.49 | 0.6858 | -772.0 | -651.1 | |
| 0.00 | 1.79 | 0.00 | 1.20 | -16.82 | 202.88 | -35.55 | 124.62 | 0.6785 | -556.0 | -545.2 | |
| 0.00 | 0.81 | 0.00 | 0.54 | -16.50 | 202.83 | -35.59 | 124.17 | 0.6768 | -421.0 | -408.8 | |
| 23.01 | 110.67 | 15.38 | 73.83 | -15.94 | 202.79 | -35.63 | 123.44 | 0.6735 | -935.1 | -630.1 | |
| 2.60 | -41.00 | 1.74 | -41.00 | -16.34 | 202.67 | -35.75 | 123.86 | 0.6775 | -638.1 | 999999 | |
| 1.97 | -41.00 | 1.31 | -41.00 | -15.22 | 202.82 | -35.60 | 122.53 | 0.6685 | -883.6 | 999999 | |
| 0.00 | 3.13 | 0.00 | 2.14 | -17.86 | 202.25 | -36.18 | 125.45 | 0.6920 | -756.0 | -652.7 | |
| 5.37 | -41.00 | 3.61 | -41.00 | -16.23 | 202.50 | -35.92 | 123.59 | 0.6785 | -620.8 | 999999 | |
| 0.00 | 0.45 | 0.00 | 0.31 | -18.18 | 201.97 | -36.45 | 125.65 | 0.6969 | -499.0 | -454.2 | |
| 0.00 | 1.16 | 0.00 | 0.80 | -17.98 | 201.94 | -36.48 | 125.38 | 0.6959 | -515.0 | -447.5 | |
| 0.00 | 0.63 | 0.00 | 0.44 | -18.62 | 201.46 | -36.96 | 125.81 | 0.7049 | -739.0 | -663.6 | |
| 0.00 | 1.34 | 0.00 | 0.94 | -18.50 | 201.25 | -37.17 | 125.52 | 0.7063 | -619.0 | -545.7 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -18.62 | 201.02 | -37.40 | 125.50 | 0.7094 | -468.0 | -399.7 | |
| 0.00 | 1.52 | 0.00 | 1.02 | -14.57 | 201.51 | -36.91 | 120.77 | 0.6788 | -50.0 | -112.6 | |
| 0.00 | 0.54 | 0.00 | 0.38 | -19.13 | 200.11 | -38.31 | 125.48 | 0.7216 | -481.0 | -532.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |