Abstract
The zonal mean state of the atmosphere in the Northern Hemisphere in winter is
determined by the temperature at the Earth’s surface and by two potential vorticity
(PV) anomalies (defined as that part of the PV field that induces a wind field)
centred over the North Pole: one in the upper troposphere/lower stratosphere
(UTLS), extending to the Subtropics, and the other over the polar cap in the lower
to middle stratosphere. Isentropic PV inversion demonstrates that the UTLS PV
anomaly induces themain part of the zonalmean wind in the troposphere, including
the subtropical jet stream, while the stratospheric PV anomaly induces the polar
night stratospheric jet. The stratospheric PV anomaly has a greater amplitude and
extends further downwards if the Arctic Oscillation (AO) index is positive. Also, the
UTLS PV anomaly has a slightly larger amplitude if the AO index is positive, but
the meridional PV gradient in the Subtropics that is associated with this anomaly is
greatest when the AO index is negative, resulting in a stronger subtropical jet when
the AO index is negative. PV inversion translates the UTLS PV anomaly into a wind
anomaly and a static stability anomaly. The resulting differences in the vertical wind
shear and in the Brunt–V¨ais¨al¨a frequency between the two AO phases show a larger
baroclinicity in the extratropics when the AO index is positive. This explains why
more extratropical cyclones are observed when the AO index is positive
Original language | English |
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Pages (from-to) | 20-29 |
Number of pages | 10 |
Journal | Quarterly Journal of the Royal Meteorological Society |
Volume | 136 |
DOIs | |
Publication status | Published - 2010 |