A Satellite Survey

of

Cloud Cover and Water Vapor

In the

Southwestern U.S.A. and Northern Mexico

 

 

 

 

 

 

 

A study conducted for:

 

The CELT Project

 

by

 

D. André Erasmus

Certified Consulting Meteorologist

 

and

 

C.A. van Staden

 

 

30 June, 2002

 

 


                                                            EXECUTIVE SUMMARY

 

 

Cloud cover and water vapor conditions in the southwestern U.S.A. and northern Mexico have been surveyed using fifty-eight months of meteorological satellite observations made between July 1993 and September 1999. An aerial mapping of cloud and water vapor has resulted in the identification of preferred areas for locating optical and infra-red telescopes. Additionally, based on the findings of the aerial survey, fifteen existing and potential telescope sites were selected for further analysis. Cloud cover and water vapor conditions at these sites were compared and the sites ranked in terms of their observing quality.

 

Defining observing conditions as photometric, spectroscopic and unsuitable for astronomy, respectively, the frequency of occurrence of these conditions were determined from satellite observations of cloud cover. The clearest sites are located along the spine of the Baja peninsula and into southern California between about 29oN and 33oN on mountain peaks above the temperature inversion layer. A steep gradient of cloudiness is observed along the coast where coastal cloud and fog are trapped below the inversion layer. Further inland, moving from west to east over the continent, a significant increase in cloudiness is observed. For example, at about 33oN, traversing Arizona from west (115oW) to east (109oW), there is a 15% decrease in the clear fraction.

 

 

 

 

 

                                                            ACKNOWLEDGEMENTS

 

This study was funded by the CELT project (University of California and California Institute of Technology), Cerro-Tololo Inter-American Observatory, University of Tokyo and European Southern Observatories. Also acknowledged for their support are: Observatorio Astrónomico Nacional San Pedro Mártir, Submillimeter Telescope Observatory (Mt. Graham) and Instituto de Astronomía Universidad Nacional Autónoma de México and the South African Astronomical Observatory.

 


TABLE OF CONTENTS

 

 

Section                                                           Topic                                                              Page

 

                   Executive Summary                                                                                        i

 

1.                Introduction                                                                                                      1

 

2.                The Meteorology and Climatology of the Study Area                                 3

 

3.                Preliminary Site Selection                                                                             6

 

4.                The Data                                                                                                        12

                   4.1       Satellite data                                                                                     12

                   4.2       Rawinsonde data                                                                              14

                   4.3       Topography data                                                                               15

                   4.4       Definitions of seasons and day/night divisions                             16

 

5.                Methodology                                                                                                  18

                   5.1       Conversion of radiance to brightness temperature                       19

                   5.2       Conversion of 6.7µm brightness temperature to UTH                  19

                   5.3       Computation of precipitable water vapor                                       20

                   5.4       Cloud detection and classification                                                  23

 

                                                                                                      

 


1.         Introduction

 

The University of California and the California Institute of Technology have initiated and are undertaking the California Extremely Large Telescope (CELT) project which aims to build a 30-m diameter ground-based telescope for astronomy at visible and infrared wavelengths (Nelson and Mast, 1999; Nelson, 2000). In support of this project, a survey of the southwestern USA and northern Mexico has been carried out to identify possible telescope sites and to assess their quality in terms of critical astronomical observing quality indicators. In a study conducted for Cerro Tololo Inter-American Observatory (CTIO) and the University of Tokyo to evaluate sites in northern Chile, cloud cover and water vapor parameters derived from meteorological satellite data were used to quantify observing conditions (Erasmus and van Staden, 2001).

 

A similar approach has been taken in this study of the southwestern U.S.A and northern Mexico. Firstly, the aerial distribution of cloud cover and water vapor over the area of interest was mapped quantitatively so that preferred areas could be identified. Based on this analysis, fifteen sites were selected for further analysis and comparison. The 15 sites include the best potential telescope sites and a number of existing observatory sites. Some existing observatories have independent records and measurements of site quality. These have been related to the satellite observations in order to validate the evaluation and ranking of site quality based on the satellite data analysis.

 

The study area covers 18oN to 40oN and 96oW to 124oW (Figure 1). It has numerous mountain peaks with altitude, shape and orientation potentially suitable for locating a large telescope. The area includes several developed telescope sites such as Mt. Graham, Kitt Peak, Palomar Mountain and San Pedro Martir.

 

Given the size of the area and the large number of possible sites to be considered, a survey method that can map cloud cover and water vapor quantitatively over the entire area leading to the identification of a limited number of good sites is needed. Additionally, the individual sites thus identified need to be compared and ranked objectively in terms of their quality. The data set must also be long enough to describe the climatology of the area (and the sites) and allow for the assessment of diurnal, seasonal and inter-annual variability.



Meteorological satellites monitor cloud cover and water vapor over large areas with a temporal, spatial and radiometric resolution that is suitable for such a survey (Figure 2). An important feature of satellite data is that these provide a consistent measurement over a field of view so that a reliable comparison of sub-regions can be made. The spatial (~10km) and temporal (3 hours) resolution of the observations also ensures that measurements are representative of conditions at particular sites and that the diurnal moisture and cloud cover cycle is resolved. Satellite data archives now consist of directly comparable measurements (consistent from one satellite to another) over extended periods (more than five years). This allows for an evaluation of observing conditions over a reasonably long time base-line. By referencing the period of satellite data against other climate data with a longer time base-line, an assessment can be made of the climatological representativeness of the study period.


 

 


Figure 2.  Full earth-disk view of the GOES-8 satellite at 11:45UT on October 25, 2000. Left, infra-red window channel (10.7µm) and right, water vapor channel (6.7µm).

 

 

This report presents the results of the survey described above. An overview of the meteorology and climatology of the study area and data period is provided in section 2. Using basic topographic and climatological criteria, a preliminary list of sites was compiled. Section 3 contains this information. Details on the satellite and other data used in the study are provided in section 4. The methodology used to derive cloud cover and water vapor parameters from the satellite data is outlined in section 5. The analysis performed and results obtained are presented in section 6. This includes an assessment of how cloud cover and water vapor conditions in the study period compare with long-term means, trends and variability (sections 6.1 and 6.2), quantitative mapping of cloud cover and water vapor conditions over the study area (section 6.3), site selection (section 6.4) and the objective comparison of cloud cover and water vapor at the 15 selected sites (sections 6.5 and 6.6).

 


2.         The Meteorology and Climatology of the Study Area

 

The southwestern U.S.A. and northern Mexico are located in the latitude region where air, lifted into the upper troposphere along the inter-tropical convergence zone and transported polewards, descends again to the surface. This descending air produces a semi-permanent region of high pressure between about 25oN and 35oN. The descending air is dry since the moisture it carried aloft over the equator has precipitated. As it descends, it is also compressed and warmed adiabatically. Consequently, the sub-tropical high pressure area is generally cloud free. At some height above the surface the descending air encounters air near the surface which is cooler. At this boundary, the normally observed decrease in temperature with height in the atmosphere is reversed. The temperature inversion layer, due to its thermal stability characteristics, prevents air near the surface moving upwards beyond the inversion base. Moisture and dust are therefore trapped below the inversion layer. The height of the inversion layer depends largely on the temperature of the surface. A warm surface promotes the formation of convective eddies above the ground, particularly in the day time, and this lifts the inversion height. At inland locations, therefore, the inversion height tends to be elevated in summer. At coastal locations the cool ocean surface has a moderating effect in summer with the result that the inversion height exhibits small diurnal and seasonal fluctuations.

 

The region of high pressure in the sub-tropics moves north in the summer and south in the winter. In winter, this southward movement allows mid-latitude cyclones moving from west to east over the Pacific Ocean to take a more southerly track. This causes the northern part of the study area to experience moist and cloudy conditions in the winter. In summer, as the center of the subtropical high pressure migrates northwards, the southern part of the study area comes under tropical influence. In the extreme south this would include Tropical storms and cyclones. Areas east of the continental divide are influenced by moisture that is circulated by the Bermuda High off the Gulf of Mexico. Moisture from this source is the fuel for much of the summer thunderstorm activity in these areas. Locations further west come under the influence of the southwest Monsoon which transports moisture from the Pacific over the southwestern U.S.A. and parts of Mexico.

 

Inter-annual variations in moisture and cloud cover are also observed over the region. This variability is controlled to a significant degree by El Niño - Southern Oscillation (ENSO) events. ENSO is a non-periodic inter-annual oscillation in the atmospheric and oceanic conditions that occurs over the tropical Pacific Ocean. Under normal or typical conditions, the weather of the southeastern Pacific is dominated by the strong, semi-permanent south Pacific Anticyclone (high pressure) which gives rise to persistent easterly winds along the Equator between the Americas and the dateline. Under these conditions, strong upwelling is encouraged in the ocean off the west coast of South America producing cold sea surface temperatures. The cold water is transported into the tropics by the combined effect of ocean currents and surface drag exerted by the trade winds. This cold water reduces evaporation rates and also stabilizes the lowest layers of the atmosphere in the Tropical eastern Pacific Ocean. In the north Pacific, the Polar Jet Stream maintains its integrity thus steering winter-time cyclonic storms along a favored track centered between northern California and the Canadian border. The cold phase of ENSO known as La Niña is simply an intensification of these “normal” conditions.

 

Every two to seven years, with irregular periodicity, an anomalous warming of the sea surface occurs in the Tropical eastern Pacific Ocean. This warming coincides with a decrease in the strength of the south Pacific high and consequently a decrease in the strength of trade winds and also in the amount of upwelling. This anomaly, which usually lasts from 12 to 18 months has become known as El Niño (the warm phase of ENSO) and directly affects the whole of the tropical and equatorial south Pacific Ocean. Indirect effects are felt over the entire Pacific basin including the southwestern U.S.A and northern Mexico. In the northern Pacific the Polar jet stream weakens and takes a more northerly track while the Subtropical jet strengthens. This tends to steer winter storms along two tracks - one northerly track into Canada and one southerly track into central and southern California. This enhances winter-time moist and cloudy conditions in southern California, northern Mexico, Arizona, New Mexico and, to a lesser extent, Nevada, Colorado and Utah. Conversely, more northerly locations (Oregon, Washington, Idaho and Wyoming) experience a drier winter (Figure 3). 

 

The effect of El Niño on Summer-time moisture and cloud is less clear. The strong El Niños of 1982 and 1991 produced more humid summers in Arizona. During some El Niño years the onset of the Summer Monsoon was delayed and summers were drier than normal. According to Reynolds et al (1999), in the Great Basin area of the western United States, above normal precipitation was recorded during El Niño years in 81% of the cases for the period April to October. Significant droughts in the Great Basin such as that of 1989 coincided with a La Niña event.

 

Given the above information on climate variability within the study area, it is important to characterize the long-term representativeness of the study period. An analysis of the climate during the study period is presented in section 6.2. A summary of ENSO events between 1993 and 1999, the period of satellite data coverage, is presented here. Table 1 and Figure 4 show that ENSO events ranged from strong El Niño to strong La Niña conditions during the study period. The average SOI for the study period is -0.6 which is near normal but slightly biased towards the warm phase of ENSO. Based on the discussion above, this consideration of ENSO conditions suggests that moisture conditions over the study area as a whole would be near normal or slightly more moist than normal during the study period. A more detailed assessment may be found in section 6.2.

 

Table 1. Summary of ENSO conditions for the study period, July 1993 to September 1999.

 

PERIOD

ENSO CONDITIONS

January 1993 – November 1993

Weak El Niño

December 1993 – February 1994

Normal

March 1994 – November 1994

Weak El Niño

December 1994 – November 1995

Normal

December 1995 – February 1997

La Niña

March 1997 – April 1998

Strong El Niño

May 1998 – April 1999

Strong La Niña

May 1999 – September 1999

Normal

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 


Figure 4. Southern Oscillation Index (SOI), pressure anomaly at Tahiti minus pressure anomaly at Darwin, normalized and Niño region 1+2 (0oS – 10oS, 80oW – 90oW) sea surface temperature anomaly (oC) for the period 1980-2000. Positive SOI values indicate a La Niña and negative values an El Niño. Source: Climate Prediction Center, NOAA, (http://www. elnino.noaa.gov/).


3.         Preliminary Site Selection

 

As a starting point for site selection, a list of sites was compiled based on precipitation climatology and topography (primarily suitable site elevation). It is important to note that the preliminary list was intended as a point of departure in the site selection process. Other sites were added as these became known or were later identified following the area analysis.

 

Figures 5 and 6 show the mean annual precipitation distribution maps for the SW USA and Mexico. The minimum precipitation area extends from about 37oS at the California-Nevada border, more-or-less southwards to the Mexico border. In northern Mexico the dry zone extends into Baja and Sonora. Precipitation enhancement occurs along the Sierra Madre Occidental but dry pockets are observed between the west coast and the cordillera even as far south as 20oS. Another dry area is observed east of the Sierra Madre Occidental due to a rain shadow effect created by the mountains. This area is flat and low lying.

 

In terms of topography, telescope sites need to be located on suitably elevated mountain tops. Elevation is needed to ensure that the site lies above the temperature inversion layer that exists at the interface between air that is sinking from the tropopause level (~ 12km) and air that is near the surface. As explained in section 2, locations above the height of the inversion layer tend to remain free of moisture and/or dust from the surface. The height of the inversion layer varies diurnally, seasonally and geographically but, in order that a site is above the inversion layer as frequently as possible, sites should be as high as possible. For the purposes of compiling the preliminary list of sites, a minimum altitude of 2000m was specified in most instances. Exceptions were made in the case of some existing sites and sites close to the ocean where the inversion layer height is considerably lower. Where two or more sites are found in close proximity, preference was given to the higher site.

 

The considerations noted above have led to the preliminary list of sites shown in Tables 2 - 5 and Figures 7 - 10. In selecting these sites, lack of road access did not rule out a site. Other factors that may eventually rule out a site such as geologic stability, mining activity or light pollution were not taken into account in the compilation of the preliminary list. These factors were given consideration before the final list of sites was decided upon (see section 6.4). On completion of the aerial analysis of cloud cover and water vapor (section 6.3), preferred areas with the clearest skies and lowest moisture conditions were identified. These areas were examined and other sites, not necessarily on the preliminary list, were added to the pool from which the final list of potential sites was compiled.

 


Figure 5. Mean annual precipitation for the southwestern USA for the period 1961-1990. (National Atlas of the United States® , www-atlas.usgs.gov/)

Figure 6. Mean annual precipitation for Mexico.

(Perry-Castañeda Library Map Collection, www.lib.utexas.edu/maps)