| 1. | It refers to mean solar time at the meridian of Greenwich, England.
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| 2. | The definition of the second in mean solar time, however, is unchanged.
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| 3. | In traditional astronomical usage, civil time was mean solar time reckoned from midnight.
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| 4. | Most later equation clocks, made in the 18th Century, directly display solar time.
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| 5. | The times above are based on local solar time, rather than standard time.
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| 6. | This resulted in leap second adjustments to keep UTC synchronised with solar time.
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| 7. | This discrepancy aggregates and causes a difference between clock time and solar time.
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| 8. | This aggregates to the angular equivalent of mean solar time + 12 hours.
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| 9. | If the gear ratios are correct, the clock shows solar time.
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| 10. | The "'equation of time "'describes the discrepancy between two kinds of solar time.
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