the impact of solar cycle on the dry sand skin temperature at ponce de leon beach
DESCRIPTION
The impact of solar cycle on the dry sand skin temperature at Ponce de Leon Beach . Jeremy Fimat. Motivations. Skin temperature (T s ) is important to remote sensing (satellite). T s connected to airflow in dune environment through radiative fluxes (energy budget). - PowerPoint PPT PresentationTRANSCRIPT
The impact of solar cycle on the dry sand
skin temperature at Ponce de Leon Beach
Jeremy Fimat
Motivations
• Skin temperature (Ts) is important to remote sensing (satellite).
• Ts connected to airflow in dune environment through radiative fluxes (energy budget).
• Fluxes impact the wind flow and atmospheric stability.
• Biological effects: Turtles hatchlings.
“The Denuded Beach”
Transect
From water’s edge to dune crest (East-to-West)
Methods• Skin temperature measured with an IR
thermometer.• Every 3 feet.
When
• Data collected over two days and two different periods of the day:- 23 June 2010: 10am – 3pm
6 transects.- 30 June 2010: 6pm – 9pm
3 transects.
ZONE 2 ZONE 1ZONE 3 ZONE 0
Wet sandDamp sand“Beach”: Dry sand
The 4 zones of the transect / 23 June
Dune
Transect
8am 4pm 12am
Sand temperature diurnal variation
R.J. Stathers, June 1984Time1pm 9pm
D
ry sa
nd te
mpe
ratu
re (
C)
• Surface energy budget: energy balance under ideal conditions (e.g., clear sky).
• 4 energy fluxes at skin surface:– Rn: Net radiation= incoming – outgoing radiation– SH: Sensible heat (Air). – GH: Ground heat flux.– LH: Latent heat: water vapor flux.
Diurnal skin temperature changes (ΔT)
Responses
Surface Energy Budget: for dry sand in early-morning (8am)
Sand surface
Rn
SH
GH
Surface Energy Budget: for dry sand at mid-morning (10am)
Sand surface
Rn
SH
GH
Surface Energy Budget: for dry sand at solar peak (1pm-2pm)
Sand surface
Rn
SH
GH
Surface Energy Budget: for dry sand at mid-afternoon (3/4pm)
Sand surface
Rn
SH
GH
Surface Energy Budget: for dry sand in early evening (6pm)
Sand surface
Rn SH
GH
Surface Energy Budget: for dry sand in late evening (9pm)
Sand surface
RnSH
GH
Expectations for ΔT
• ΔT = T an hour – T at the previous hour.• ΔT>0 = warming.• ΔT<0 = cooling.• An important ΔT in early morning (10am).• ΔT decreasing until solar peak.• ΔT = 0 in early afternoon.• ΔT increasing until sunset (9pm).
Local solar radiation on 23 June 2010
2:30 PM
1 PM
ZONE 2 ZONE 1ZONE 3 ZONE 0
Wet sandDamp sand“Beach”: Dry sand
The 4 zones of the transect / 23 June
Dune
Transect
The Beach Zone: ZONE 2 / 23 June
ZONE 2 ZONE 1ZONE 3 ZONE 0
Wet sandDamp sand“Beach”: Dry sand
The 4 zones of the transect / 30 June
Dune
Transect
The Beach Zone: ZONE 2 / 30 June
Observed ΔT with timeBeach Zone (ZONE 2)
Decreased warming: ΔT less positive.
Increased cooling: ΔT more negative.
Average ΔT = +8.3 FAverage ΔT = +6 F
Average ΔT = +3.3 FAverage ΔT = +0.4 F
Average ΔT = -9.5 F
Average ΔT = -11.4 F
Elevation sun angle with time
Sunrise Sunset
ΔT > 0 : Warming ΔT < 0 : Cooling
Decreased warmingIncreased cooling
• Maximum warming rate during mid-morning.• Maximum cooling rate during the evening.• Equilibrium after solar peak.• Dry sand skin temperature is correlated to
slope of solar elevation angle.• Governed by surface energy budget.
Conclusion/Summary: Dry sand / Beach Zone (ZONE 2)
Questions ? Next: Erik Mackay