Assessment of Radiometer Calibration with GPS Radio Occultation for the Mirata Cubesat Mission Anne D
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New Capabilities for All-Weather Microwave Atmospheric Sensing Using Cubesats and Constellations
SSC18-II-07 New Capabilities for All-Weather Microwave Atmospheric Sensing Using CubeSats and Constellations W. Blackwell, K. Clark, D. Cousins, D. Crompton, A. Cunningham, M. Diliberto, L. Fuhrman, R. Leslie, I. Osaretin, and S. Michael MIT Lincoln Laboratory [email protected] ABSTRACT Three MIT Lincoln Laboratory nanosatellite missions flying microwave radiometers for high-resolution atmospheric sensing are in varying stages of development. Microwave instrumentation is particularly well suited for implementation on a very small satellite, as the sensor requirements for power, pointing, and spatial resolution (aperture size) can be accommodated by a nanosatellite platform. The Microsized Microwave Atmospheric Satellite Version 2a (MicroMAS-2a), launched on January 11, 2018 and has demonstrated temperature sounding using channels near 118 GHz and humidity sounding using channels near 183 GHz. A second MicroMAS-2 flight unit (MicroMAS-2b) will be launched in Fall 2018 as part of ELANA-XX. The Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats (TROPICS) mission was selected by NASA in 2016 as part of the Earth Venture–Instrument (EVI-3) program. The overarching goal for TROPICS is to provide nearly all-weather observations of 3-D temperature and humidity, as well as cloud ice and precipitation horizontal structure, at high temporal resolution to conduct high-value science investigations of tropical cyclones. TROPICS will provide rapid-refresh microwave measurements (median refresh rate of approximately 40 minutes for the baseline mission) over the tropics that can be used to observe the thermodynamics of the troposphere and precipitation structure for storm systems at the mesoscale and synoptic scale over the entire storm lifecycle. -
Software Developement Tools Introduction to Software Building
Software Developement Tools Introduction to software building SED & friends Outline 1. an example 2. what is software building? 3. tools 4. about CMake SED & friends – Introduction to software building 2 1 an example SED & friends – Introduction to software building 3 - non-portability: works only on a Unix systems, with mpicc shortcut and MPI libraries and headers installed in standard directories - every build, we compile all files - 0 level: hit the following line: mpicc -Wall -o heat par heat par.c heat.c mat utils.c -lm - 0.1 level: write a script (bash, csh, Zsh, ...) • drawbacks: Example • we want to build the parallel program solving heat equation: SED & friends – Introduction to software building 4 - non-portability: works only on a Unix systems, with mpicc shortcut and MPI libraries and headers installed in standard directories - every build, we compile all files - 0.1 level: write a script (bash, csh, Zsh, ...) • drawbacks: Example • we want to build the parallel program solving heat equation: - 0 level: hit the following line: mpicc -Wall -o heat par heat par.c heat.c mat utils.c -lm SED & friends – Introduction to software building 4 - non-portability: works only on a Unix systems, with mpicc shortcut and MPI libraries and headers installed in standard directories - every build, we compile all files • drawbacks: Example • we want to build the parallel program solving heat equation: - 0 level: hit the following line: mpicc -Wall -o heat par heat par.c heat.c mat utils.c -lm - 0.1 level: write a script (bash, csh, Zsh, ...) SED -
Passive Microwave Radiometer Channel Selection Based on Cloud and Precipitation Information Content Estimation
475 Passive Microwave Radiometer Channel Selection Based on Cloud and Precipitation Information Content Estimation Sabatino Di Michele and Peter Bauer Research Department Submitted to Q. J. Royal Meteor. Soc. July 2005 Series: ECMWF Technical Memoranda A full list of ECMWF Publications can be found on our web site under: http://www.ecmwf.int/publications/ Contact: [email protected] c Copyright 2005 European Centre for Medium-Range Weather Forecasts Shinfield Park, Reading, RG2 9AX, England Literary and scientific copyrights belong to ECMWF and are reserved in all countries. This publication is not to be reprinted or translated in whole or in part without the written permission of the Director. Appropriate non-commercial use will normally be granted under the condition that reference is made to ECMWF. The information within this publication is given in good faith and considered to be true, but ECMWF accepts no liability for error, omission and for loss or damage arising from its use. Microwave Channel Selection from Precipitation Information Content Abstract The information content of microwave frequencies between 5 and 200 GHz for rain, snow and cloud wa- ter retrievals over ocean and land surfaces was evaluated using optimal estimation theory. The study was based on large datasets representative of summer and winter meteorological conditions over North Amer- ica, Europe, Central Africa, South America and the Atlantic obtained from short-range forecasts with the operational ECMWF model. The information content was traded off against noise that is mainly produced by geophysical variables such as surface emissivity, land surface skin temperature, atmospheric temperature and moisture. The estimation of the required error statistics was based on ECMWF model forecast error statistics. -
Unix Tools 2
Unix Tools 2 Jeff Freymueller Outline § Variables as a collec9on of words § Making basic output and input § A sampler of unix tools: remote login, text processing, slicing and dicing § ssh (secure shell – use a remote computer!) § grep (“get regular expression”) § awk (a text processing language) § sed (“stream editor”) § tr (translator) § A smorgasbord of examples Variables as a collec9on of words § The shell treats variables as a collec9on of words § set files = ( file1 file2 file3 ) § This sets the variable files to have 3 “words” § If you want the whole variable, access it with $files § If you want just the second word, use $files[2] § The shell doesn’t count characters, only words Basic output: echo and cat § echo string § Writes a line to standard output containing the text string. This can be one or more words, and can include references to variables. § echo “Opening files” § echo “working on week $week” § echo –n “no carriage return at the end of this” § cat file § Sends the contents of a file to standard output Input, Output, Pipes § Output to file, vs. append to file. § > filename creates or overwrites the file filename § >> filename appends output to file filename § Take input from file, or from “inline input” § < filename take all input from file filename § <<STRING take input from the current file, using all lines un9l you get to the label STRING (see next slide for example) § Use a pipe § date | awk '{print $1}' Example of “inline input” gpsdisp << END • Many programs, especially Okmok2002-2010.disp Okmok2002-2010.vec older ones, interac9vely y prompt you to enter input Okmok2002-2010.gmtvec • You can automate (or self- y Okmok2002-2010.newdisp document) this by using << Okmok2002_mod.stacov • Standard input is set to the 5 contents of this file 5 Okmok2010.stacov between << END and END 5 • You can use any label, not 5 just “END”. -
Useful Commands in Linux and Other Tools for Quality Control
Useful commands in Linux and other tools for quality control Ignacio Aguilar INIA Uruguay 05-2018 Unix Basic Commands pwd show working directory ls list files in working directory ll as before but with more information mkdir d make a directory d cd d change to directory d Copy and moving commands To copy file cp /home/user/is . To copy file directory cp –r /home/folder . to move file aa into bb in folder test mv aa ./test/bb To delete rm yy delete the file yy rm –r xx delete the folder xx Redirections & pipe Redirection useful to read/write from file !! aa < bb program aa reads from file bb blupf90 < in aa > bb program aa write in file bb blupf90 < in > log Redirections & pipe “|” similar to redirection but instead to write to a file, passes content as input to other command tee copy standard input to standard output and save in a file echo copy stream to standard output Example: program blupf90 reads name of parameter file and writes output in terminal and in file log echo par.b90 | blupf90 | tee blup.log Other popular commands head file print first 10 lines list file page-by-page tail file print last 10 lines less file list file line-by-line or page-by-page wc –l file count lines grep text file find lines that contains text cat file1 fiel2 concatenate files sort sort file cut cuts specific columns join join lines of two files on specific columns paste paste lines of two file expand replace TAB with spaces uniq retain unique lines on a sorted file head / tail $ head pedigree.txt 1 0 0 2 0 0 3 0 0 4 0 0 5 0 0 6 0 0 7 0 0 8 0 0 9 0 0 10 -
Instruments for Earth Science Measurements
NASA SBIR 2004 Phase I Solicitation E1 Instruments for Earth Science Measurements NASA's Earth Science Enterprise (ESE) is studying how our global environment is changing. Using the unique perspective available from space and airborne platforms, NASA is observing, documenting, and assessing large- scale environmental processes with emphasis on atmospheric composition, climate, carbon cycle and ecosystems, the Earth’s surface and interior, the water and energy cycles, and weather. A major objective of the ESE instrument development programs is to implement science measurement capabilities with small or more affordable spacecraft so development programs can meet multiple mission needs and therefore, make the best use of limited resources. The rapid development of small, low cost remote sensing and in situ instruments is essential to achieving this objective. Consequently, the objective of the Instruments for Earth Science Measurements SBIR topic is to develop and demonstrate instrument component and subsystem technologies that reduce the risk, cost, size, and development time of Earth observing instruments, and enable new Earth observation measurements. The following subtopics are concomitant with this objective and are organized by measurement technique. Subtopics E1.01 Passive Optics Lead Center: LaRC Participating Center(s): ARC, GSFC The following technologies are of interest to NASA in the remote sensing subtopic “passive optics.” Passive optical remote sensing generally requires that deployed devices have large apertures and large throughput. NASA is interested primarily in instrument technologies suitable for aircraft or space flight platforms, and these inherently also prefer low mass, low power, fast measurement times, and a high degree of robustness to survive vibrations in flight or at launch. -
Basic Plotting Codes in R
The Basics of R for Windows We will use the data set timetrial.repeated.dat to learn some basic code in R for Windows. Commands will be shown in a different font, e.g., read.table, after the command line prompt, shown here as >. After you open R, type your commands after the prompt in what is called the Console window. Do not type the prompt, just the command. R stores the variables you create in a working directory. From the File menu, you need to first change the working directory to the directory where your data are stored. 1. Reading in data files Download the data file from www.biostat.umn.edu/~lynn/correlated.html to your local disk directory, go to File -> Change Directory to select that directory, and then read the data in: > contact = read.table(file="timetrial.repeated.dat", header=T) Note: if the first row of the data file had data instead of variable names, you would need to use header=F in the read.table command. Now you have named the data set contact, which you can then see in R just by typing its name: > contact or you can look at, for example, just the first 10 rows of the data set: > contact[1:10,] time sex age shape trial subj 1 2.68 M 31 Box 1 1 2 4.14 M 31 Box 2 1 3 7.22 M 31 Box 3 1 4 8.00 M 31 Box 4 1 5 7.09 M 30 Box 1 2 6 8.55 M 30 Box 2 2 7 8.79 M 30 Box 3 2 8 9.68 M 30 Box 4 2 9 6.05 M 30 Box 1 3 10 6.25 M 30 Box 2 3 This data set has 6 variables, one each in a column, where sex and shape are character valued. -
PS TEXT EDIT Reference Manual Is Designed to Give You a Complete Is About Overview of TEDIT
Information Management Technology Library PS TEXT EDIT™ Reference Manual Abstract This manual describes PS TEXT EDIT, a multi-screen block mode text editor. It provides a complete overview of the product and instructions for using each command. Part Number 058059 Tandem Computers Incorporated Document History Edition Part Number Product Version OS Version Date First Edition 82550 A00 TEDIT B20 GUARDIAN 90 B20 October 1985 (Preliminary) Second Edition 82550 B00 TEDIT B30 GUARDIAN 90 B30 April 1986 Update 1 82242 TEDIT C00 GUARDIAN 90 C00 November 1987 Third Edition 058059 TEDIT C00 GUARDIAN 90 C00 July 1991 Note The second edition of this manual was reformatted in July 1991; no changes were made to the manual’s content at that time. New editions incorporate any updates issued since the previous edition. Copyright All rights reserved. No part of this document may be reproduced in any form, including photocopying or translation to another language, without the prior written consent of Tandem Computers Incorporated. Copyright 1991 Tandem Computers Incorporated. Contents What This Book Is About xvii Who Should Use This Book xvii How to Use This Book xvii Where to Go for More Information xix What’s New in This Update xx Section 1 Introduction to TEDIT What Is PS TEXT EDIT? 1-1 TEDIT Features 1-1 TEDIT Commands 1-2 Using TEDIT Commands 1-3 Terminals and TEDIT 1-3 Starting TEDIT 1-4 Section 2 TEDIT Topics Overview 2-1 Understanding Syntax 2-2 Note About the Examples in This Book 2-3 BALANCED-EXPRESSION 2-5 CHARACTER 2-9 058059 Tandem Computers -
N€WS 'RELEASE NATIONAL AERONAUTICS and SPACE Admln ISTRATION 400 MARYLAND AVENUE, SW, WASHINGTON 25, D.C
https://ntrs.nasa.gov/search.jsp?R=19630002483 2020-03-11T16:50:02+00:00Z b " N€WS 'RELEASE NATIONAL AERONAUTICS AND SPACE ADMlN ISTRATION 400 MARYLAND AVENUE, SW, WASHINGTON 25, D.C. TELEPHONES WORTH 2-4155-WORTH. 3-1110 RELEASE NO. 62-182 MARINER SPACECRAFT Mariner 2, the second of a series of spacecraft designed for planetary exploration,- will be launched within a few days (no earlier than August 17) from the Atlantic Missile Range, Cape Canaveral, Florida, by the National Aeronautics and Space Administration. Mariner 1, launched at 4:21 a.m. (EST) on July 22, 1962 from AMR, was destroyed by the Range Safety Officer after about 290 seconds of flight because of a deviation from the planned flight path. Measures have been taken to correct the difficulties experienced in the Mariner 1 launch. These measures include a more rigorous checkout of the Atlas rate beacon and revision of the data editing equation. The data editing equation Is designed as a guard against acceptance of faulty databy the ground guidance equipment. The Mariner 2 spacecraft and its mission are identical to the first Mariner. Mariner 2 will carry six experiments. Two of these instruments, infrared and microwave radiometers, will make measurements at close range as Mariner 2 flys by Venus and communicate this in€ormation over an interplanetary distance of 36 million miles, Four other experiments on the spacecraft -- a magnetometer, ion chamber and particle flux detector, cosmic dust detector and solar plasma spectrometer -- will gather Information on interplantetary phenomena during the trip to Venus and in the vicinity of the planet. -
Attitudes Toward Disability
School of Psychological Science Attitudes Toward Disability: The Relationship Between Attitudes Toward Disability and Frequency of Interaction with People with Disabilities (PWD) # Jennifer Kim, Taylor Locke, Emily Reed, Jackie Yates, Nicholas Zike, Mariah Es?ll, BridgeBe Graham, Erika Frandrup, Kathleen Bogart, PhD, Sam Logan, PhD, Chris?na Hospodar Introduc)on Methods Con)nued Conclusion The social and medical models of disability are sets of underlying assump?ons explaining Parcipants Connued Suppor?ng our hypothesis, the medical and social models par?ally mediated the people's beliefs about the causes and implicaons of disability. • 7.9% iden?fied as Hispanic/Lano & 91.5% did not iden?fy as Hispanic/Lano relaonship between contact and atudes towards PWD. • 2.6% iden?fied as Black/African American, 1.7% iden?fied as American Indian or Alaska • Compared to the social model, the medical model was more strongly associated • The medical model is the predominant model in the United States that is associated Nave, 23.3% iden?fied as Asian, 2.2% iden?fied as Nave Hawaiian or Pacific Islander, with contact and atudes. with the belief that disability is an undesirable status that needs to be cured (Darling & 76.7% iden?fied as White, & 2.1% iden?fied as Other • This suggests that more contact with PWD can help decrease medical model beliefs Heckert, 2010). This model focuses on the diagnosis, treatment and curave efforts • Average frequency of contact was about once a month in general, but may be slightly less effec?ve at promo?ng the social model beliefs. related to disability. -
An Assessment of Rain “Contamination” in ARM Two
An assessment of rain “contamination” in ARM two-channel microwave radiometer measurements Roger Marchand1, Casey Wall1*, Wei Zhao1 and Maria Cadeddu2 1University of Washington, 2Argonne National Laboratory, *Presenting Author Case 1 Case 3 Motivation! ? !! ✔ ? � ✔ 5000 wet-window flag (open/covered) ! Microwave radiometers (MWRs) are the most commonly used and wet-window flag (open/covered) 1500 3000 accurate instruments ARM has to retrieve cloud liquid water path. open MWR open MWR Unfortunately, MWR data are not easily used in precipitating conditions. 1000 500 There are two reasons for this:" 5000 ) ) 2 1500 " 2 1. The measurements are “contaminated” by water on the MWR radome." 3000 covered! covered! MWR MWR 2. Precipitating particles can scatter microwave radiation, yet traditional 1000 500 MWR retrievals neglect scattering." 5000 " 1500 "We designed an experiment that alleviates the “wet radome” problem. 3000 1000 500 5000 The Experiment! 1500 !! 3000 500 ! Two MWRs were operated side by side in a “scanning” or tip-cal mode. Path (g/m Water Liquid 1000 Liquid Water Path (g/m Path Water Liquid One MWR was placed under a cover that kept the radome dry while still 5000 permitting measurements away from zenith (photograph below). The 1500 other MWR was operated normally, with the radome exposed to the sky. 3000 We refer to these as the “covered” and “open” MWRs, respectively. 1000 500 Coincident measurements from the 17.8 18.2 18.6 19 19.4 19.8 covered and open MWRs are 17.5 18 18.5 19 compared to estimate contamination Hours (UTC) Hours (UTC) Case 2 due to a wet radome. -
Evidence of Diurnal Variations of Titan's Near-Surface Temperature
EPSC Abstracts Vol. 14, EPSC2020-618, 2020 https://doi.org/10.5194/epsc2020-618 Europlanet Science Congress 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Evidence of diurnal variations of Titan’s near-surface temperature and of a cooling effect of the northern seas from the Cassini radar/radiometer Alice Le Gall1,2, Léa Bonnefoy1,3, Robin Sultana4, Michael Janssen5, Ralph Lorenz6, and Tetsuya Tokano7 1LATMOS/IPSL, UVSQ, Université Paris-Saclay, CNRS, Sorbonne Université 2Institut Universitaire de France (IUF), Paris, France 3LESIA, Observatoire de Paris/Université PSL, CNRS, Sorbonne Université, Université Paris-Diderot, Meudon, France 4IPAG, Université Grenoble Alpes, CNRS, Grenoble, France 5Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 6Johns Hopkins Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD, USA 7Institut für Geophysik und Meteorologie, Universität zu Köln, Cologne, Germany At first order, the physical temperature of Titan’s surface can be regarded as nearly constant and predictable. Due to the low incident solar flux reaching its surface (1/1000 of what Earth receives) and the high thermal inertia of its atmosphere, diurnal, seasonal (including latitudinal) and altitudinal variations of temperature are limited as well as the effect of surface albedo (Lorenz et al., 1999). Voyager 1 radio-occultation measurements indeed show no diurnal effect and point to lapse rates in the lower atmosphere smaller than 1.5 K/km (McKay et al 1997). Voyager infrared observations indicate a pole-to-equator temperature contrast of 2-3 K (Flasar et al., 1981; 1998). The Cassini mission (2004-2017) somewhat confirmed these predictions and first measurements.