Halogen Occultation Experiment (HALOE L2 and L3 Version 19)
General Info
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Instrument on board the UARS satellite which used solar occultation technique to measure global stratospheric and mesospheric profiles of pressure, temperature, O3, HCl, HF, CH4, H2O, NO, NO2 and aerosol extinction. Approx. 30 sunset and sunrise profiles per day between 80S and 80N. October 1991 to 1994. Data are level 2 products i.e. profiles at actual measurement location and not interpolated in horizontal. Data are version 19. Access permission required for Level 2 data so that PI can monitor usage of data. Level 3 data is public.
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Introduction
The Halogen Occultation Experiment (HALOE) is one of 10 instruments aboard the Upper Research Satellite (UARS). The HALOE instrument was built by an instrument team based at NASA Langley and launched on the UARS on 12th September 1991. Data collection began on 11th October 1991 until 21st November 2005. The Principal Investigator (PI) is Dr James M. Russell III. The HALOE experiment uses solar occultation to measure vertical profiles of ozone (O3), hydrogen chloride (HCl), Hydrogen Fluoride (HF), methane (CH4), water vapour (H2O), nitric oxide (NO), nitrogen dioxide (NO2), aerosol extinction, and temperature versus pressure with an instantaneous vertical field of view of 1.6 km at the Earth limb. The instrument achieves near-global coverage with measurements sweeping between high latitudes in one hemisphere and high latitudes in the other over a period of between 2 and 6 weeks. The latitude range covered by the instrument varies over the course of the year between 80°S and 80°N. The maximum northerly and southerly latitudes occur in spring and autumn in the few weeks either side of the equinoxes. The range of altitude of the measurements depends on the channel being used, but measurements cover the stratosphere and lower mesosphere and, in the case of the nitric oxide channel, extend into the lower thermosphere. HALOE studies the dynamics of polar and other atmospheric regions using the tracers, HF, CH4 and H2O. Studying the trends in HCl and HF will help distinguish the relative importance of anthropogenic versus natural chlorine sources and analyse in detail the development and recovery of the Antarctic ozone hole. Additional studies are intended to identify and assess stratosphere-troposphere exchange. The BADC holds HALOE data at level 2 (uninterpolated profiles at measurement locations), version 19 for the period 11th Ocotber 1991 to 21st November 2005. The BADC also holds the HALOE level 3A version 19 data spanning the time period from 11th October 1991 through 21st December 2000. HALOE L3 data is public. Updates through to September 24, 2001 are available directly from GSFC NASA. The HALOE level 3A data are vertical profiles of methane (CH4), hydrogen chloride (HCl), hydrogen fluoride (HF), nitric oxide (NO), nitrogen dioxide (NO2), water vapor (H2O), ozone (O3), temperature (TEMP), and aerosol extinction (AEXTCH4, AEXTHCL, AEXTHF and AEXTNO), interpolated onto a standard set of vertical levels evenly spaced in pressure, and onto standard times (level 3AT) and standard latitudes (level 3AL). The vertical scan range is from about 10 to 65 km, and the vertical resolution is approximately 2.5 km between pressure levels. Access Restrictions
File format
The data are provided in an IEEE Unix binary format. A HALOE-L2 guide is available to help you retrieving the HALOE Level 2 data. Similarly, a HALOE-L3 guide is available to help you retrieving the HALOE Level 3 data. Software to read HALOE Level 2 and software to read Haloe Level 3 are provided to read the data files. HALOE version 19 data in netCDF format is also available for download from the Haloe website at NASA. Documentation, Links to further information and references
The BADC provides several documents to help you use this dataset. These include the full set of documentation produced by the instrument team at NASA Langley, as well as a help file written at the BADC which contains an overview of the instrument, measurement techniques and the species measured, including details of coverage, resolution and data quality. You may browse the HALOE Homepage from which you may also download the data in netCDF format (compressed with Gzip). The HALOE version 19 Image Selector is also available from this website. The HALOE L3A Version 19 data are originally available from the GSFC NASA. The HALOE instrument is described in Russell et al. (1993) J. Geophys. Res. 98 D6, pp. 10777 - 10797. Some early results from HALOE are described in the UARS special issue of the Journal of Atmospheric Science (vol 51 no. 20). We provide a list of references to papers using HALOE data and a list of references to other UARS paper. A continuously updated list of references is available from the HALOE NASA webpage. Citation
Who to contact
For general queries about these pages or about browsing the data, you should contact the BADC support line. For further information about the data or the instrument contact the HALOE Principal Investigator James Russell or his team at NASA Langley. Prof. John Harries at Imperial College, London is a UK Co-Investigator. | |||
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HALOE Level 2 was acquired as is in the late 1990's and was updated monthly until 2005. HALOE-L3 data was acquired as is in 2000.
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Data quality controlled by NASA.
Please the BADC HALOE Data Helpfile for details (http://badc.nerc.ac.uk/data/haloe/haloehelp.html)
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