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Mutual Amplification Between Upper and LowerLevel Cyclonic Potential Vorticity in the Deepening of a

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Title: Mutual Amplification Between Upper and LowerLevel Cyclonic Potential Vorticity in the Deepening of a


1
Mutual Amplification Between Upper and
Lower-Level Cyclonic Potential Vorticity in the
Deepening of a Extratropical Cyclone A Case Study
  • Holly A. Anderson
  • Synoptic-Dynamic Meteorology
  • Dr. Cunningham
  • December 6, 2007

2
Objectives
  • An extratropical cyclone that formed on November
    20, 2006 off the east coast of the United States
    is analyzed within a PV and isentropic framework.
  • This project seeks to describe the synoptic
    conditions leading to the development of the
    extratropical cyclone, as well as provide a study
    of the evolution of the associated potential
    vorticity fields as the upper-level cyclonic PV
    anomalies and the surface level cyclone mutually
    affect each other.

3
Case Study November 21-22, 2006
  • A developing coastal extratropical storm brought
    freezing temperatures, heavy rains, frozen
    precipitation, and erosion to the east coast.
  • Knocked down power lines and caused power outages
    to many along the east coast
  • Rainfall totals
  • Georgetown, DE 1.93 (49 mm) 22 Nov
  • Newark, NJ 1.26 (32 mm) 23 Nov
  • Kennedy Airport, NY - 1.56 (40 mm) 23 Nov
  • Shoreham, NY 2.83 (72 mm) 23 Nov
  • Bridgeport, CT 1.84 (47 mm) 23 Nov
  • Hingham, MA 4.76 (121 mm) 24 Nov

4
November 21, 2006
  • Snow flurries were reported by the National
    Weather Service as far south as central Florida
    in Orange, Lake, Seminole, and Volusia counties
    Florida as the state endured unusually early cold
    temperatures.

5
Charleston, South Carolina
  • The first record of thundersnow in local history.
  • Earliest winter season calendar date on which
    snow has been reported at KCHS.

NWS PNS - http//www.erh.noaa.gov/chs/text/PNSCHS_
11222006.txt
6
21 November 2006 12Z
7
Isentropic Potential Vorticity A Review
  • IPV is conserved following 3-D, adiabatic,
    inviscid flow along an isentrope. By plotting
    Ertel PV on an isentropic surface, we can see a
    conserved quantity along a surface of another
    conserved quantity.
  • Values of PV less than 2 PVU are typically
    tropospheric. Stratospheric values of PV are
    typically greater than 4 PVU, where 1 PVU 10-6
    m2s-1Kkg-1 (Bresky and Colucci, 1996).
  • For this study, the tropopause is defined by the
    1.5 PVU surface.
  • PV values of 1.5-4 PVU define the dynamic
    tropopause (Bresky and Colucci, 1996).

8
Data and Methodology
  • NCAR Computational and Information Systems
    Laboratory (CISL) Data for Atmospheric and
    Geosciences Research
  • NCEP Eta model data
  • 40 km resolution
  • 3 hour time intervals
  • 26 pressure levels
  • Analyzed in both Unidata Integrated Data Viewer
    (IDV) and GrADS
  • For this project, plan view plots of IPV at the
    310K isentrope were plotted.
  • In addition, PV cross-sections were calculated
    using centered finite differencing at pressure
    levels from 1000-50 hPa.
  • By looking at plan views and vertical
    cross-sections, the interaction between the
    upper-level PV anomalies and the surface cyclone
    can be studied. The evolution in the position of
    the dynamic tropopause can also be noted.

9
21 November 00Z
10
21 November 12Z
11
22 November 00Z
12
22 November 12Z
13
23 November 00Z
14
Isotachs (shaded) and Heights (contours)
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21
PV and Cyclogenesis
  • Positive PV on the 310K surface indicate the
    positive PV field in the upper-troposphere.
  • The upper anomaly induces cyclonic motion that
    extends down into the troposphere.
  • The upper level cyclonic motion acts to amplify
    the cyclonic motion at the surface, strengthening
    the surface cyclone.
  • In turn, the surface cyclone amplifies the
    upper-level cyclonic motion.
  • As long as they tilt westward with height,
    cyclonic motions at upper and lower levels
    mutually amplify one another in a feedback
    mechanism.
  • Therefore, we expect to see higher PV values in
    the upper atmosphere as the surface cyclone
    deepens.
  • Tropopause depression is noted by upper-level PV
    anomalies.

22
21 November 00Z
  • Isobars indicate the cyclone is forming.
  • The upper PV field is to the west of the
    low-level cyclone.

23
21 November 12Z
  • The upper PV anomaly blob is tightening as the
    MSLP isobars tighten, indicating that both fields
    are strengthening and amplifying each other. The
    IPV at 310K has obtained a value of 5.5 PVU and
    is directly west of the surface cyclone.

24
21 November 12Z
  • Location of the cross-section from 32N, 85W to
    32N, 71W

25
21 November 12Z
  • As this cross-section cuts through the center of
    the cyclone, we see cyclonic motion from the
    meridional isotachs.
  • Isentropes also bend upwards into the positive PV
    anomaly.
  • Tropopause undulations are also seen.
  • Tropopausal values of PV are shown close to the
    surface.

26
22 November 00Z
  • The PV blob is advecting southeastward. The
    highest PVU value is 6 PVU, well into
    stratospheric values. The cyclone has achieved a
    low pressure of less than 1005 hPa.

27
22 November 00Z
  • Location of the cross-section from 27N, 84W to
    27N, 76W

28
22 November 00Z
  • Cyclonic motion is seen surrounding this PV
    anomaly.
  • The tropopause is low in the atmosphere, at
    approximately 500-550 hPa. This means
    stratospheric values are the lowest. This
    corresponds to what we expect as the cyclone
    intensifies.

29
22 November 12Z
  • The PV blob is at its tightest gradient, as is
    the surface low. The surface low pressure is less
    than 1002 hPa.
  • The highest PV values are southwest of the
    surface cyclone.

30
22 November 12Z
  • Location of the cross-section from 31N, 81W to
    31N, 78W

31
22 November 12Z
  • The 310K isentrope is clearly within
    stratospheric values and is found around the 400
    hPa level.
  • The tropopause is higher at this time, at
    approximately 475 hPa.
  • The low-level PV anomaly is most likely due to
    diabatic heating at the surface.

32
23 November 00Z
  • By 00Z on the 23 November, the upper-PV blob is
    becoming less tilted westward with height. The
    IPV field at 310K has weakened considerably. PV
    values have lowered to more tropospheric values.
    Likewise, the cyclone has diminished in strength,
    as shown by higher pressure values and a smaller
    pressure gradient.

33
23 November 00Z
  • Location of the cross-section from 81W, 31N to
    77W, 31N through the southwestern part of the
    surface cyclone

34
23 November 00Z
  • Stratospheric values are back to the 225-250 hPa
    level.
  • The isentropes are also vertically stacked.
  • Cyclonic motion is visible from the isotachs of
    meridional wind.
  • PV of 1.5 PVU are at higher pressures, indicating
    the dynamic troposphere is very close to the
    ground.

35
23 November 12Z
  • The low continues to move off to the northeast,
    tracking alongside the east coast. PV values
    continue to diminish and the blob weakens as
    the PV anomaly is no longer tilted westward with
    height.

36
24 November 00Z
  • The PV blob decays to tropospheric values as
    the weakening cyclone moves northeastward off the
    coast.
  • At this point, the upper-level PV blob is
    beginning to tilt westward with height once
    again. As the cyclone moves off the coast, it
    will bomb and strengthen once again.

37
Concluding Remarks
  • Upper-level PV anomalies, noted by cyclonic
    motion, are amplified by lower-level cyclonic
    motion when they are tilted westward with height.
  • We can see a clear relationship between the
    strength of the surface cyclone and the PV values
    of upper-level anomalies.
  • Though this cyclone was not the strongest at this
    time, we can see how the upper-level PV anomalies
    and the surface low mutually amplified one
    another until they became stacked vertically with
    height and therefore decayed.

38
References
  • Jonathan E. Martin, 2006 Mid-Latitude
    Atmospheric Dynamics A First Course, The
    University of Wisconsin-Madison.
  • Davis, C. A., and K. A. Emanuel, 1991 Potential
    vorticity diagnostics of cyclogenesis. Mon. Wea.
    Rev., 119, 1929-1953.
  • Bresky, Wayne C. and Stephen J. Colucci, 1996 A
    Forecast and Analyzed Cyclogenesis Event
    Diagnosed with Potential vorticity. Mon. Wea.
    Rev., 124, 22272244.
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