Lapse rate: Refers to the rate of temperature change with
height in the atmosphere. A steep lapse rate is one in which the
environmental temperature decreases rapidly with height. The steeper
the environmental lapse rate, the more potentially unstable is
the atmosphere.
Let LR(e) = Environmental lapse rate.
Let LR(p) = Parcel lapse rate.
Let LR(da) = Dry adiabatic lapse rate (dry ascent).
Let LR(ma) = Moist adiabatic lapse rate (saturated
ascent).
For dry/unsaturated convection, LR(p) = LR(da).
For moist/saturated convection, LR(p) = LR(ma).
An evaluation of moisture is critical
for determining the potential for convection, severe weather,
and heavy rainfall. Thunderstorms can develop in an area of significant
ambient or inflow moisture. In evaluating moisture, consider the
surface to 700 mb dewpoints, 1000-500 mb precipitable water (PW),
the K index, and moisture convergence. During the warm season,
rough threshold values (and higher values representing better
potential) for heavy rain include:
These are rough numbers and heavy rain or severe weather may still occur at values below these, especially if significant forcing is present, or during the cool season.
The Total Totals Index consists of two
components, the Vertical Totals (VT) and the Cross Totals (CT).
The VT represents static stability or the lapse rate between 850
and 500 mb. The CT includes the 850 mb dewpoint. As a result,
TT accounts for both static stability and 850 mb moisture, but
would be unrepresentative in situations where the low-level moisture
resides below the 850 mb level. In addition, convection may be
inhibited despite a high TT value if a significant capping inversion
is present.
TT
= VT + CT
VT = T(850 mb) - T(500 mb)
CT = Td(850 mb) - T(500 mb)
in degrees C, where T represents
temperature at the indicated level and Td represents dewpoint
temperature.
VT = 40 is close to dry adiabatic for the 850-500 mb layer. However,
VT generally will be much less, with values around 26 or more
representing sufficient static instability (without regard to
moisture) for thunderstorm occurrence. CT > 18 often is necessary
for convection, but it is the combined Total Totals Index that
is most important.
TT
= T(850 mb) + Td(850 mb) - 2[T(500 mb)] in
degrees C.
TT = 45 to
50: Thunderstorms
possible.
TT = 50 to
55: Thunderstorms
more likely, possibly severe.
TT = 55 to
60: Severe thunderstorms
most likely.
These parameters assess the contribution of middle-level lapse rate to convective instability. A steep 700-500 mb lapse rate overtop low-level moisture is quite favorable for strong/severe convection including microbursts and hail. The DTI measures the temperature difference between two mandatory pressure levels (often 700-500 mb). The DTI is similar to the Vertical Totals.
10.2 deg C/km: | Dry adiabatic lapse rate (700-500 mb) |
DTI = 26 deg C in warm season: | Dry adiabatic lapse rate (700-500 mb) |
6.5 C/km for 700 mb temp = 0 C: | Moist adiabatic lapse rate (700-500 mb) |
6.0 C/km for 700 mb temp = +5 C: | Moist adiabatic lapse rate (700-500 mb) |
5.6 C/km for 700 mb temp = +10 C: | Moist adiabatic lapse rate (700-500 mb) |
DTI = 18 C in warm season: | Moist adiabatic lapse rate (700-500 mb) |
The K index is a measure of thunderstorm
potential based on the vertical temperature lapse rate, and the
amount and vertical extent of low-level moisture in the atmosphere.
K = T(850 mb) + Td(850 mb) -
T(500 mb) - DD(700 mb)
in degrees C, where T represents
temperature, Td represents dewpoint temperature, and DD represents
dewpoint depression at the indicated level.
K below 30: | Thunderstorms with heavy rain or severe weather possible (see note below). |
K over 30: | Better potential for thunderstorms with heavy rain. |
K = 40: | Best potential for thunderstorms with very heavy rain. |
The LI is a commonly utilized measure
of stability which measures the difference between a lifted parcel's
temperature at 500 mb and the environmental temperature at 500
mb. It incorporates moisture and lapse rate (static stability)
into one number, which is less vulnerable to observations at individual
pressure levels. However, LI values do depend on the level from
which a parcel is lifted, and rally cannot account for details
in th environmental temperature curve above the LCL and below
500 mb. LI was originally intended to utilize average moisture
and temperature properties within the planetary boundary layer.
LI = T(500 mb envir) - T(500
mb parcel)
in degrees C, where T (500 mb
envir) represents the 500 mb environmental temperature and T (500
mb parcel) is the rising air parcel's 500 mb temperature.
LI over 0: | Stable but weak convection possible for LI = 1-3 if strong lifting is present. |
LI = 0 to -3: | Marginally unstable. |
LI = -3 to -6: | Moderately unstable. |
LI = -6 to -9: | Very unstable. |
LI below -9: | Extremely unstable. |
The SI is based on the properties of
the 850 and 500 mb levels. The SI is calculated by lifting a parcel
dry adiabatically from 850 mb to its LCL, then moist adiabatically
to 500 mb, and comparing the parcel versus environmental 500 mb
temperatures similar to the LI. The SI may be better than the
LI in showing instability aloft given a shallow low-level cool
airmass north of a frontal boundary. However, the SI is an unrepresentative
index and inferior to the LI in showing instability if the low-level
moisture does not extend up to the 850 mb level.
SI
= T(500 mb envir) - T(500 mb parcel) in degrees C.
SI over 0: | Stable, but weak convection possible for SI = 1-2 if strong lifting is present. |
SI = 0 to -3: | Moderately unstable. |
SI = -4 to -6: | Very unstable. |
SI below -6: | Extremely unstable. |
Generally,
SI values will not be quite as unstable as LI ( cept for
the case of shallow low-level cool air discussed above).
The DCI attempts to combine the properties
of equivalent potential temperature (Qe) at 850 mb with instability.
DCI
= T(850 mb) + Td(850 mb) - LI(sfc-500 mb)
in degrees C, where LI represents the lifted index value from
the surface to 500 mb.
This is a relatively new index. Therefore, no definitive critical
values have been determined. However, DCI values of roughly 30
or higher indicate the potential for strong thunderstorms. Ridge
axes of DCI may be even more important and a location for thunderstorm
development given the presence of upward motion.
The SWEAT Index evaluates the potential
for severe weather by combining several parameters into one index.
These parameters include low-level moisture (850 mb dewpoint),
instability (Total Totals Index), lower and middle-level (850
and 500 mb) wind speeds, and warm air advection (veering between
850 and 500 mb). Therefore, an attempt is made to incorporate
kinematic and thermodynamic information into one index. As such,
the SWEAT index should be utilized to assess severe weather potential,
not ordinary thunderstorm potential.
SWEAT
= 12 [Td(850 mb)] + 20 (TT - 49) + 2 (f8) + f5 + 125 (S + 0.2)
where TT represents the total
totals index value, f8 and f5 represent the 850 mb and 500 mb
wind speed in knots, respectively, and S = sin (500 mb minus 850
mb wind direction), i.e., the sine of the angle between the 500
and 850 mb wind directions (the shear term).
The last term in the equation (the shear term) is set to zero
if any of the following criteria are not met: 1) 850 mb wind direction
ranges from 130 to 250 degrees, 2) 500 mb wind direction ranges
from 210 to 310 degrees, 3) 500 mb wind direction minus the 850
mb wind direction is a positive number, and 4) both the 850 and
500 mb wind speeds are at least 15 kts. No term in the equation
may be negative; if so, that term is set to zero.
SWEAT over 300: Potential for severe
thunderstorms.
SWEAT over 400: Potential for tornadoes.
These are guidance values developed
by the U.S. Air Force. Severe storms may still be possible for
SWEAT values of 250-300 if strong lifting is present. In addition,
tornadoes may occur with SWEAT values below 400, especially if
convective cell and boundary interactions increase the local shear
which would not be resolved in this index. The SWEAT value can
increase significantly during the day, so low values based on
1200 UTC data may be unrepresentative if substantial changes in
moisture, stability, and/or wind shear occur during the day. Finally,
as with all indices, the SWEAT only indicates the potential for
convection. There must still be sufficient forcing for upward
motion to release the instability before thunderstorms can develop.
CAPE assumes Parcel Theory, in that 1)
a rising parcel exhibits no environmental entrainment, 2)
the parcel rises (moist) adiabatically, 3) all precipitation
falls out of the parcel (no water loading), and 4) the
parcel pressure is equal to the environmental pressure at each
level. Parcel Theory can have significant errors, especially for
large parcel displacements, at cloud edges, and for significant
water loading. However, the method often works quite well in the
undiluted core of a thunderstorm updraft.
CAPE represents the amount of buoyant energy available to accelerate
a parcel vertically, or the amount of work a parcel does on the
environment. CAPE is the positive area on a sounding between the
parcel's assumed ascent along a moist adiabat and the environmental
temperature curve from the level of free convection (LFC) to the
equilibrium level (EL). The greater the temperature difference
between the warmer parcel and the cooler environment, the greater
the CAPE and updraft acceleration to produce strong convection.
EL
CAPE = g { [(Tparcel - Tenvir) / Tenvir]
dz
LFC
in Joules/kg. The "{"
symbol here represents a vertical integration between the LFC
(level of free convection, above which the parcel is warmer than
the environment, i.e., the parcel is positively buoyant and will
rise) and the EL (equilibrium level, below which the parcel is
warmer than the environment).
CAPE below 0: | Stable. |
CAPE = 0 to 1000: | Marginally unstable. |
CAPE = 1000 to 2500: | Moderately unstable. |
CAPE = 2500 to 3500: | Very unstable. |
CAPE above 3500-4000: | Extremely unstable. |
CIN represents the amount of negative
buoyant energy available to inhibit or suppress upward vertical
acceleration, or the amount of work the environment must do on
the parcel to raise the parcel to its LFC. CIN basically is the
opposite of CAPE, and represents the negative energy area (B-)
on the sounding where the parcel temperature is cooler than that
of the environment. The smaller (larger) the CIN is, the weaker
(stronger) must be the amount of synoptic and especially mesoscale
forced lift to bring the parcel to its LFC. High CIN values in
the presence of little or no lift can cap or suppress convective
development, despite possibly high CAPE values. Remember, CAPE
is the "available potential" energy. That energy must
be released to become "kinetic" energy to produce thunderstorms.
The LSI measures the ability of a stable
layer to inhibit low-level parcel ascent. If the cap is strong
enough, then deep moist convection will be suppressed, even if
the airmass is very unstable. However, a cap allows the low-level
moisture and temperature to increase which ultimately enhances
severe weather potential for those stronger convective cells that
are able to break the cap. Therefore, thunderstorms which develop
rapidly within or near an area of significant capping likely will
become severe. Conversely, the lack of a lid allows many storms
to develop which then compete for the available moisture and storm-relative
inflow.
LSI =
Qsw - Qwmax
where Qsw is the maximum saturated Qw (wet bulb potential temperature)
between the surface and 500 mb, and Qwmax is the maximum Qw in
the lowest 100 mb of the atmosphere.
LSI below 2: | Deep convection generally should not be inhibited. |
LSI above 2: | Deep convection may be suppressed unless sufficient heating, moisture convergence, and/or forced lift overcomes the cap. |
The BRN usually is a decent indicator
of convective storm type within given environments. It incorporates
buoyant energy (CAPE) and the vertical shear of the horizontal
wind, both of which are critical factors in determining storm
development, evolution, and organization.
BRN = CAPE / [0.5
(U2)]
where U is a measure of the vertical
wind shear in the 0-6 km layer AGL, and U2 simply means U squared,
i.e., U taken to the second power. BRN is a dimensionless number.
BRN below 10: | Strong vertical wind shear and weak CAPE. The shear may be too strong given the weak buoyancy to develop sustained convective updrafts. However, given sufficient forcing, thunderstorms may still develop; if so, rotating supercells could evolve given the high shear. |
BRN = 10 to 45: | Associated with supercell development. |
BRN over 50: | Relatively weak vertical wind shear and high CAPE which suggests multicellular thunderstorm development is most likely. |
While BRN can be useful in assessing While BRN can be useful in assessing the potential for supercell and middle-level mesocyclone development, it is less suited to assess low-level mesocyclone and tornado potential. Conversely, BRN shear may be more useful in differentiating between those supercells that will and those that will not produce tornadoes, although BRN shear still cannot be used independently for this purpose as storm-scale interactions are crucial for tornado development.
BRN shear = 0.5 (Uavg)2
in m2/s2, where Uavg, the magnitude difference between the 0-6 km mean wind in the lowest 0.5 km, is squared (i.e., taken to the second power).
BRN shear = 25 to 100 | Associated with tornadic supercells (assuming supercells form on a given day). |
However, values from 25 to 50 can be associated with tornadic and non-tornadic storms, with values near and above 50 more likely to be associated with tornadoes. Nevertheless, BRN shear, which is sensitive to low-level winds and is a function of he degree and depth of the wind shear, tends to be higher for tornadic storms than for non-tornadic storms as lower BRN shear values reflect weaker environmental wind shear. Also, favorable BRN shear values combined with favorable 500 mb storm-relative winds (see section below) are more likely to be associated with tornadic supercells.
Middle-level (represented well by the 500 mb level) storm-relative (S-R) winds also may be useful to help differentiate between tornadic and non-tornadic supercells within the overall environment, assuming supercells will form on a given day. Middle-level S-R winds are important in order to create a balance between the low-level storm inflow along the forward front flank baroclinic zone and the low-level outflow associated with the rear flank downdraft. If very weak S-R winds are present, a large amount of precipitation tends to wrap around the mesocyclone leading to the generation of excessive rain-cooled outflow along the low-level rear flank of the storm. This cool air then undercuts the middle-level mesocyclone and disrupts the low-level circulation. On the other hand, if middle-level S-R winds are very strong, then the middle-level flow may remove too much precipitation downwind from the mesocyclone, inhibiting the development of enough rain-cooled outflow (i.e., downdraft) along the rear flank to help focus convergence and generate baroclinic vorticity. Between these two extremes exists a balance where the rear flank downdraft is pronounced but balanced by significant low-level S-R flow into the system. S-R winds at 500 mb can be calculated from subtracting the observed or forecasted storm motion from the observed or forecasted 500 mb wind speeds.
500 mb S-R winds = 16 kts (8 m/s) | Lower limit for tornadic supercells. |
500 mb S-R winds = 40 kts (20 m/s) | Approximate upper limit for tornadic supercells |
Tornado potential is highest when 500
mb S-R winds are relatively high and low-level storm inflow can
be enhanced through boundaries, mesolows, etc. Strong low-level
inflow and convergence enhances the generation of baroclinically-induced
horizontal vorticity along the forward front downdraft boundary.
This vorticity then funnels into the weak echo region where it
is tilted vertically and stretched rapidly upward (due to the
middle-level mesocyclone). This process can enhance the low-level
mesocyclone resulting in tornado development or maintenance.
Storm-relative (S-R) helicity (Hs-r)
is an estimate of a thunderstorm's potential to acquire a rotating
updraft given an environmental vertical wind shear profile, assuming
thunderstorms are able to develop. It integrates the effects of
S-R winds and the horizontal vorticity (generated by vertical
shear of the horizontal wind) within the inflow layer of a storm.
A S-R wind is the wind that a thunderstorm actually "feels"
as the storm moves through the environment. It is different from
a true ground-relative (G-R) wind, except for a stationary storm
whereby a S-R and G-R wind are equivalent. S-R helicity is proportional
to the area "swept out" by the S-R wind vectors between
two levels on a hodograph.
Hs-r = {
(v - c) . W dz
where v = actual ground-relative
wind vector, c = storm motion vector, (v - c) = storm-relative
wind vector, W = horizontal vorticity vector, the dot
"." represents a mathematical dot product, and
the "{" represents a vertical integration over
a specified depth (usually the lowest 2 or 3 km of the atmosphere).
Units are m2/s2 (i.e., meters squared divided by seconds squared).
Hs-r = 150: | The approximate threshold for supercell development. |
Hs-r = 150 to 299: | Weak tornadoes (F0 and F1) possible. |
Hs-r = 300 to 449: | Strong tornadoes (F2 and F3) possible. |
Hs-r over 450: | Violent tornadoes (F4 and F5) possible. |
CAPE and storm-relative (S-R) helicity
(Hs-r) are both very important in the formation of a strongly
rotating convective updraft. CAPE represents the amount of buoyant
energy available, while S-R helicity incorporates the effects
of environmental vertical wind shear and storm motion on thunderstorm
type and evolution. An intense rotating updraft can form with
relatively weak CAPE if the vertical wind shear and storm-relative
inflow are strong. On the other hand, relatively low S-R helicity
usually can be compensated by high instability to produce a rotating
updraft. The EHI attempts to combine CAPE and S-R helicity into
one index to assess the potential for supercell and mesocyclone
development. High EHI values represent an environment possessing
high CAPE and/or high S-R helicity.
EHI = [CAPE
(Hs-r)] / 160,000
EHI is a dimensionless
number.
The full operational utility of the
EHI is not yet completely known. In addition, there is some discrepancy
as to what the minimum threshold is for severe thunderstorms and
tornadoes. However, general threshold values are given below.
EHI below 1.0: | Supercells and tornadoes unlikely in most cases, but be aware of convective interactions and shear zones that could make EHI values unrepresentative. |
EHI = 1.0 to 2.0: | Supercells and tornadoes are possible but usually tornadoes are not of violent or long-lived. Can get non-supercell/shear vorticy tornadoes near the leading edge of bow echoes/LEWPS. |
EHI = 2.0 to 2.4: | Supercells more likely and mesocyclone-induced tornadoes possible. |
EHI = 2.5 to 2.9: | Mesocyclone-induced supercellular tornadoes more likely. |
EHI = 3.0 to 3.9: | Strong mesocyclone-induced tornadoes (F2 and F3) possible. |
EHI over 4.0: | Violent mesocyclone-induced tornadoes (F4 and F5) possible. |
Wet bulb temperature (Tw) represents
the lowest temperature a volume of air at a constant pressure
can be cooled to by evaporating water into it. Its value falls
between the dry bulb (actual air) temperature and dewpoint. To
compute Tw at a particular level (pressure) on a sounding, lift
up a dry adiabat and saturation mixing ratio line to the lifting
condensation level (LCL; i.e., where parcel saturation is achieved,
in other words, cloud base) then come down the moist adiabat to
the original pressure and read the Tw value (Note: coming back
down to 1000 mb represents the wet bulb potential temperature,
Qw). The NWS Louisville Science
and Technology Page is created and maintained by Ted Funk,
The height of the wet bulb zero is that level on the sounding
whereby the lowest temperature attainable (given the ambient temperature
and dewpoint at that level) through isobaric evaporation of water
is zero degrees C, i.e. Tw = 0 C at this level.
In general, WBZ heights from
5,000 to 12,000 ft AGL are associated
with hail at the ground. The potential for large hail is highest
for WBZ heights of 7,000
to 10,000 ft AGL, with rapidly diminishing hail size below
6,000 and above 11,000 ft AGL. Above 11,000 ft, hail is less common since
it has a smaller depth in which to form and may melt before reaching
the ground due to a significant warm cloud layer below. However,
very heavy rain may occur in these cases. WBZ values too low indicate
a shallow warm cloud depth with less warm cloud collision-coalescence
occurring to provide the necessary liquid drops and droplets to
increase hail size.
Research has suggested that a crucial factor for hail growth is
the presence of a broad region of moderate updraft (20-40 m/s),
and that hail growth typically occurs on the edges and not within
a storm's strongest updraft.
Evaluation of the sounding WBZ height and freezing level are very
important in determining whether a given environment has the potential
to produce small hail, large hail, or no hail but possibly heavy
rain. A very warm airmass/high 1000-500 mb thickness value would
contain high WBZ and freezing level heights while a significant
trough or cold air aloft would lower these heights significantly.
This also relates to the Vertically Integrated Liquid (VIL) product
on the WSR-88D. A warm airmass may mean a high "VIL of the
day" threshold for hail, while cold air aloft could mean
a much lower "VIL of the day." In other words, VIL thresholds
for hail can change daily, with a meaningful VIL value one day
being less significant another day. Thus, local studies to stratify
pertinent VIL values versus various environments are important.
For example, the parameter "VIL density" has been established
to overcome some of the shortcomings of using VIL by itself. In
short, VIL density can be used to identify those storms with high
VIL values relative to the storms' echo tops in order to assess
large hail potential.
Science and Operations Officer, NWS Louisville, KY.