J/A+A/565/A102      Mesospheric sodium properties            (Pfrommer+, 2014)

High resolution mesospheric sodium properties for adaptive optics applications. Pfrommer T., Hickson P. <Astron. Astrophys. 565, A102 (2014)> =2014A&A...565A.102P 2014A&A...565A.102P
ADC_Keywords: Earth Keywords: atmospheric effects - instrumentation: adaptive optics - site testing - methods: observational Abstract: The performance of laser guide star adaptive optics (AO) systems for large optical and infrared telescopes is acted by variability of the sodium layer, located at altitudes between 80 and 120km in the upper mesosphere and lower thermosphere. The abundance and density structure of the atomic sodium found in this region is subject to local and global weather ects, planetary and gravity waves and magnetic storms, and is variable on time scales down to tens of milliseconds, a range relevant to AO. It is therefore important to characterize the structure and dynamical evolution of the sodium region on small, as well as large spatial and temporal scales. Parameters of particular importance for AO are the mean sodium altitude, sodium layer width and the temporal power spectrum of the centroid altitude. We have conducted a three-year campaign employing a high-resolution lidar system installed on the 6-m Large Zenith Telescope (LZT) located near Vancouver, Canada. During this period, 112 nights of useful data were obtained. Description: UBC Lidar Data Conversion Programs This software may be freely distributed and used by anyone. No warranty or representations are made concerning this software, and no liability of any kind will be accepted in connection with its use. Please report any bugs to To install, cd to the directory containing this file and the source code and run $ make The binary files 'centroid', 'density' and 'fileinfo' will be generated. You can move them to a more convenient directory (eg. /usr/local/bin). Information on the lidar data format, and the use of these programs can be found in the data_format.pdf document. P. Hickson, 2014 File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fits.dat 59 134 List of FITS files fits/* . 134 Individual FITS files (total is 125Gbytes) data_format.pdf 512 927 LIDAR data format and software explanations LZTlidar-1.0f.tar 1056 1429 All files needed to read the fits files -------------------------------------------------------------------------------- Byte-by-byte Description of file: fits.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- FileName Name of the fits file in subdirectory fits 19- 23 I5 --- N [420/29545] Number of "blocks" of 50 shots of data 25- 34 A10 "YYYY-MM-DD" Start.date UTC date of observation 36- 43 A8 "h:m:s" Start.time Starting time of observation 45- 52 A8 "h:m:s" End Ending time of observation 54- 59 F6.1 Mibyte Size Size of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Thomas Pfrommer, tpfromme(at)eso.org
(End) Patricia Vannier [CDS] 09-May-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line