SDO HMI 2014-11-14 21:00:27 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.83 | 163.10 | 32.46 | 173.25 | 13.93 | 14.85 | 61.97 | 284.27 | 0.8850 | -301.6 | -149.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-14 21:00:27 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 |
| 9.29 | 34.82 | 10.59 | 39.76 | 13.01 | 17.12 | 64.25 | 283.05 | 0.9027 | -487.9 | -144.5 | |
| 0.00 | 1.63 | 0.00 | 1.78 | 12.77 | 15.77 | 62.89 | 282.87 | 0.8924 | -434.0 | -318.9 | |
| 0.00 | 0.60 | 0.00 | 0.66 | 13.16 | 15.81 | 62.94 | 283.30 | 0.8929 | -459.0 | -412.3 | |
| 0.00 | 0.60 | 0.00 | 0.65 | 12.60 | 15.55 | 62.68 | 282.69 | 0.8907 | -537.0 | -480.0 | |
| 3.95 | 53.99 | 4.40 | 59.89 | 14.27 | 16.28 | 63.41 | 284.51 | 0.8970 | -218.2 | -73.8 | |
| 4.21 | -5.00 | 4.62 | -5.00 | 14.13 | 15.94 | 63.06 | 284.38 | 0.8944 | -624.4 | 999999 | |
| 1.46 | 21.24 | 1.58 | 22.74 | 13.39 | 15.58 | 62.70 | 283.57 | 0.8912 | -463.9 | -527.9 | |
| 0.00 | 1.03 | 0.00 | 1.10 | 12.55 | 15.20 | 62.33 | 282.66 | 0.8879 | -462.0 | -511.2 | |
| 2.41 | -5.00 | 2.65 | -5.00 | 14.41 | 16.01 | 63.13 | 284.68 | 0.8951 | -759.9 | 999999 | |
| 0.00 | 1.12 | 0.00 | 1.21 | 13.79 | 15.50 | 62.62 | 284.02 | 0.8908 | -419.0 | -381.6 | |
| 2.75 | -7.00 | 2.95 | -7.00 | 13.49 | 15.23 | 62.35 | 283.71 | 0.8886 | -737.4 | 999999 | |
| 1.72 | 3.61 | 1.83 | 3.84 | 14.02 | 14.95 | 62.07 | 284.33 | 0.8867 | -577.7 | -513.9 | |
| 0.52 | 1.72 | 0.55 | 1.82 | 14.28 | 14.80 | 61.93 | 284.63 | 0.8857 | -538.5 | -437.1 | |
| 0.00 | 1.46 | 0.00 | 1.53 | 15.00 | 14.38 | 61.50 | 285.48 | 0.8828 | -557.0 | -473.1 | |
| 0.00 | 0.95 | 0.00 | 1.01 | 16.82 | 14.96 | 62.09 | 287.47 | 0.8887 | -394.0 | -352.7 | |
| 0.00 | 2.58 | 0.00 | 2.67 | 15.20 | 13.96 | 61.09 | 285.75 | 0.8797 | -711.0 | -558.6 | |
| 0.00 | 4.21 | 0.00 | 4.06 | 14.66 | 11.61 | 58.73 | 285.37 | 0.8597 | -602.0 | -516.8 | |
| 0.00 | 1.38 | 0.00 | 1.31 | 14.25 | 11.14 | 58.27 | 284.95 | 0.8553 | -139.0 | -104.9 | |
| 0.00 | 7.22 | 0.00 | 6.82 | 13.95 | 10.96 | 58.09 | 284.62 | 0.8534 | 29.0 | 6.4 | |
| 1.20 | 3.18 | 1.14 | 3.01 | 14.69 | 10.97 | 58.10 | 285.47 | 0.8542 | -722.4 | -640.3 | |
| 0.00 | 1.72 | 0.00 | 1.63 | 14.90 | 11.06 | 58.19 | 285.71 | 0.8552 | -501.0 | -474.0 | |
| 2.32 | 4.56 | 2.15 | 4.22 | 13.89 | 10.24 | 57.37 | 284.62 | 0.8470 | 631.2 | 488.0 | |
| 0.00 | 0.69 | 0.00 | 0.63 | 14.14 | 10.06 | 57.18 | 284.94 | 0.8456 | 416.0 | 367.8 | |
| 0.00 | 1.12 | 0.00 | 1.00 | 13.31 | 8.91 | 56.03 | 284.08 | 0.8342 | 341.0 | 271.3 | |
| 0.00 | 5.93 | 0.00 | 5.24 | 13.69 | 8.44 | 55.57 | 284.59 | 0.8302 | 591.0 | 433.5 | |
| 0.00 | 1.46 | 0.00 | 1.28 | 13.80 | 8.10 | 55.23 | 284.76 | 0.8271 | 655.0 | 577.6 | |
| 0.00 | 1.89 | 0.00 | 1.65 | 14.57 | 7.79 | 54.92 | 285.73 | 0.8250 | 528.0 | 422.3 | |
| 0.00 | 0.69 | 0.00 | 0.61 | 15.91 | 8.00 | 55.12 | 287.32 | 0.8286 | 406.0 | 327.9 | |
| 0.00 | 1.89 | 0.00 | 1.71 | 20.34 | 8.29 | 55.42 | 292.52 | 0.8379 | 555.0 | 373.0 | |
| 0.00 | 1.81 | 0.00 | 1.42 | 18.04 | 2.56 | 49.68 | 290.99 | 0.7788 | 626.0 | 516.4 | |
| 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. | |