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The RHUBC Campaign: Analysis of Water Vapor Profiles Eli Mlawer 1 , Jennifer Delamere 1 , Dave Turner 2 , Scott Paine 3 , Vivienne Payne 1 , Maria Caddedu 4 , Karen Cady_Pereira 1 (1) AER, Inc. ([email protected] ) (2) SSEC, Univ. Wisconsin – Madison (3) Smithsonian Astrophysical Observatory (4) Argonne National Laboratory Specifying Water Vapor Profiles During RHUBC-II The Radiative Heating in Underexplored Bands Campaign (RHUBC) Initial Evaluation of Multi-level WV Retrieval from GVRP Measurements: 9/19, 1530 UT; PWV~0.28mm Radiative cooling in the upper troposphere is dominated by water vapor in the far-IR (~300 cm -1 ). Surface spectral measurements under typical conditions (bottom panel, red) provide no information about the associated radiative processes, while those in very dry locations do (bottom, blue). Motivation: •Mid-tropospheric radiative cooling modulates vertical motions of the atmosphere Occurs primarily in water vapor absorption bands that are opaque at the surface • Approximately 40% of the OLR comes from the far-IR Need to validate water vapor absorption models in these normally opaque bands. RHUBC-II Campaign – Atmospheric Radiation Measurement Program (DOE) • Held in location with extremely low water vapor: Atacama Desert, Chile - high altitude site – Cerro Toco (5350 m) • July – November 2009 • Key Instruments Vaisala RS-92 radiosondes – ~130 launches G-band Vapor Radiometer Profiler (GVRP) – 15 channels on side of 183.3 GHz WV line SAO FTS – zenith radiance from 300-3500 GHz (resolution 3 GHz) U. Cologne HATPRO – 7 channels from 22.2 -31 GHz, 7 channels from 51-58 GHz NASA LaRC Far-IR Spectroscopy of the Troposphere (FIRST) – 100-1600 cm -1 (res. 0.6 cm -1 ) CNR (Italy) Radiation Explorer in the Far-IR (REFIR-PAD) – 100-1400 cm -1 (res. 0.5 cm -1 ) U. Wisc. Atmospheric Emitted Radiance Interferometer ( AERI) – 550-3000 cm -1 (res. 0.5 cm -1 ) Analysis of the data collected is underway Infrared Cooling Rates and Transmittances • Sondes provide an initial determination of the water vapor field above the site, but have known issues. Water vapor column amounts (PWV) measured by radiosondes during RHUBC-II. For reference, PWV for US Standard atmosphere is 14.3 mm. From Miloshevich et al. (2009), the RS92 daytime mean percentage bias relative to frost-point hygrometer measurements. This is the basis for the “Milo” correction presented below. Individual and average water vapor (right) and temperature (left) profiles measured by RHUBC-II sondes. Sonde Measurements During RHUBC-II Sonde Biases To establish baseline WV profiles for this study: • the Miloshewich adjustment is applied • a constant scaling factor is then retrieved using the GVRP channels and MonoRTM radiation code. SAO FTS FIRST The Miloshevich et al. adjustment in general improves the agreement between GVRP measurements and MonoRTM calculations. The retrieval lowers the residuals, as expected, although the most transparent channels still show residuals that cannot be eliminated by reasonable scaling of PWV. On average, the Miloshevich et al. adjustment leaves the near-surface water vapor unchanged and increases it higher up. The effect on PWV is a net increase of ~10%. The effect of the GVRP-based scaling is more variable. SAO FTS Line-by-line calculation The temperature profile used in the calculation is from the sonde and does not consider the short warmer path in the enclosure of the instrument. This causes disagreements in the opaque centers of strong water vapor lines. Publication – D. Turner and E. Mlawer, The Radiative Heating in Underexplored Bands Campaigns (RHUBC), Bull. Amer. Met Soc., in press Water vapor profile from sonde (top) Calculated MonoRTM optical depths in GVRP simulation (bottom) Calculated brightness temperatures and GVRP channel centers (top) The single- parameter retrieval reduces the PWV by 4%. (bottom) The multi- level retrieval (factors shown relative to initial guess (Milo)) also shows a decrease in PWV, but WV decreases significantly near the surface and increases at 9-13 km. Scale factors relative to sonde are also shown. The averaging kernels (left) indicate that the GVRP provides 2 pieces of information, roughly one near the surface and one ~10 km. (below) A retrieval using the sonde as initial guess/a priori demonstrates the insensitivity to these aspects of the method. Altitude (km) 25 12 6.5 5.3 Radiative Closure with Sub-millimeter FTS. (left) Measurement- model agreement in the windows is decent using the raw sonde, but a more detailed look (right) with the WV profiles detailed in the poster indicates windows with both good and not-so-good agreement. More investigation is pending.

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Page 1: The RHUBC Campaign: Analysis of Water Vapor ProfilesThe RHUBC Campaign: Analysis of Water Vapor Profiles Eli Mlawer1, Jennifer Delamere1, Dave Turner 2, Scott Paine3, Vivienne Payne1,

The RHUBC Campaign: Analysis of Water Vapor ProfilesEli Mlawer1, Jennifer Delamere1, Dave Turner2, Scott Paine3, Vivienne Payne1, Maria Caddedu4, Karen

Cady_Pereira1

(1) AER, Inc. ([email protected]) (2) SSEC, Univ. Wisconsin – Madison (3) Smithsonian Astrophysical Observatory (4) Argonne National Laboratory

Specifying Water Vapor Profiles During RHUBC-IIThe Radiative Heating in Underexplored Bands Campaign (RHUBC)

Initial Evaluation of Multi-level WV Retrieval from GVRP Measurements: 9/19, 1530 UT; PWV~0.28mm

Radiative cooling in the upper troposphere is dominated by watervapor in the far-IR (~300 cm-1). Surface spectral measurementsunder typical conditions (bottom panel, red) provide no informationabout the associated radiative processes, while those in very drylocations do (bottom, blue).

Motivation:• Mid-tropospheric radiative cooling modulates vertical motions of the atmosphere Occurs primarily in water vapor absorption bands that are opaque at the surface

• Approximately 40% of the OLR comes from the far-IRNeed to validate water vapor absorption models in these normally opaque bands.

RHUBC-II Campaign – Atmospheric Radiation Measurement Program (DOE)• Held in location with extremely low water vapor: Atacama Desert, Chile

- high altitude site – Cerro Toco (5350 m)• July – November 2009• Key Instruments Vaisala RS-92 radiosondes – ~130 launches G-band Vapor Radiometer Profiler (GVRP) – 15 channels on side of 183.3 GHz WV line SAO FTS – zenith radiance from 300-3500 GHz (resolution 3 GHz) U. Cologne HATPRO – 7 channels from 22.2 -31 GHz, 7 channels from 51-58 GHz NASA LaRC Far-IR Spectroscopy of the Troposphere (FIRST) – 100-1600 cm-1 (res. 0.6 cm-1) CNR (Italy) Radiation Explorer in the Far-IR (REFIR-PAD) – 100-1400 cm-1 (res. 0.5 cm-1) U. Wisc. Atmospheric Emitted Radiance Interferometer (AERI) – 550-3000 cm-1 (res. 0.5 cm-1)

Analysis of the data collected is underway

Infrared Cooling Rates and Transmittances • Sondes provide an initial determination of the water vapor field above the site, but have known issues.

Water vapor column amounts (PWV)

measured by radiosondes during

RHUBC-II. For reference, PWV for

US Standard atmosphere is 14.3

mm.

From Miloshevich et al. (2009), the RS92 daytime

mean percentage bias relative to frost-point

hygrometer measurements. This is the basis for the

“Milo” correction presented below.

Individual and average

water vapor (right) and

temperature (left) profiles measured by

RHUBC-II sondes.

Sonde Measurements

During RHUBC-II

Sonde Biases

To establish baseline WV profiles for this study:• the Miloshewich adjustment is applied • a constant scaling factor is then retrieved using

the GVRP channels and MonoRTM radiation code.

SAO FTSFIRST

The Miloshevich et al. adjustment in general improves the agreement

between GVRP measurements and MonoRTM calculations. The retrieval

lowers the residuals, as expected, although the most transparent

channels still show residuals that cannot be eliminated by reasonable

scaling of PWV.

On average, the Miloshevich et al.

adjustment leaves the near-surface water

vapor unchanged and increases it higher up. The effect on PWV is a net increase of ~10%.

The effect of the GVRP-based scaling is

more variable.

SAO FTSLine-by-line calculation

The temperature profileused in the calculation isfrom the sonde and doesnot consider the shortwarmer path in theenclosure of theinstrument. This causesdisagreements in theopaque centers of strongwater vapor lines.

Publication – D. Turner and E. Mlawer, The Radiative Heating in Underexplored Bands Campaigns (RHUBC), Bull. Amer. Met Soc., in press

Water vapor profile from

sonde

(top) Calculated MonoRTM

optical depths in GVRP

simulation

(bottom)Calculated brightness

temperatures and GVRP

channel centers

(top) The single-parameter retrieval reduces the PWV

by 4%.

(bottom) The multi-level retrieval (factors shown relative to initial

guess (Milo)) also shows a decrease in PWV, but WV

decreases significantly near the surface and

increases at 9-13 km. Scale factors

relative to sonde are also shown.

The averaging kernels (left) indicate that the GVRP

provides 2 pieces of information, roughly one near the surface and one ~10 km.

(below) A retrieval using the sonde as initial guess/a priori demonstrates the insensitivity

to these aspects of the method.

Alti

tude

(km

)

25

12

6.5

5.3

Radiative Closure with

Sub-millimeter FTS.

(left) Measurement-model agreement in the windows is decent using

the raw sonde, but a more detailed look (right) with the WV

profiles detailed in the poster indicates

windows with both good and not-so-good

agreement. More investigation is pending.