Workshop at NARL, Gadanki, India27-29 March 2011 - Recent Advances in Observational Studies of the Tropical Atmosphere and Ionosphere 

HAYASHI, Hiroo

KAGITANI, Masato

SHINBORI, Atsuki

TANAKA, Yoshimasa

Kyoto University Research Information Repository

TitleDevelopment of integrated analysis software of observationdata in the upper atmosphereAuthor(s)SHINBORI, Atsuki; TANAKA, Yoshimasa; KAGITANI,Masato; HAYASHI, HirooCitation (2011)Issue Date2011-03-29URL http://hdl.handle.net/2433/139543RightType PresentationTextversionauthorKyoto UniversityDevelopment of integrated analysis software of observation data in the upper atmosphere 1Atsuki Shinbori, 2Yoshimasa Tanaka, 3Masato Kagitani and 1Hiroo Hayashi, 1RISH, Kyoto University, Uji, Japan2NIPR, Tachikawa, Japan3PPARC, Tohoku Univ., Sendai, JapanMLT Seminar, NARL, India 2011/03/28-291. Contents of this talk Characteristics of TDAS（Themis Data Analysis Software suite） Introduce of UDAS (IUgonet Data Analysis Software) in the beta version1．Overview of the analysis software which has been developed in the IUGONET project2．Demonstration of the UDAS software3．Future plan and schedule of development of the UDAS software2. Overview of the TDAS/UDAS software2.1 TDAS (THEMIS Data Analysis Software suite) http://themis.ssl.berkeley.edu/ 1. The IUGONET project will provide software to analyze and visualize various kinds of ground-based observational data in our project. 2. We are developing the data analysis software on the basis of TDAS (Themis Data Analysis Software suite).3. Everybody can freely download the TDAS software from the THEMIS homepage.2. Overview of the TDAS/UDAS software2.2 Characteristics of the TDAS software-11. The data analysis software is written in IDL (Interactive Data Language), which is widely used in fields of solar and terrestrial physics.3. TDAS is adopted as data analysis software of the ERG (Energization and Radiation in Geospace) mission. Our software development is conducted in collaboration with the ERG Science Center.2. The IDL routines of TDAS enable users to easily plot and analyze various kinds of time series observation data. An example of time series plots of the MU radar observation data2. Overview of the TDAS/UDAS software2.3 Characteristics of the TDAS software-2Users can easily download the observation data from data servers and make time series plots with only 3 commands. > timespan, ‘yyyy-mm-dd’, 13, /day> thm_load_○○○> tplot, △△△User’s PCTDAS/UDAS on IDLLocal HDDLoad the tplotvariablesAutomatic data saveSSL BerkeleyTHEMIS, GBOData serverCDAWebOMNI, ACE, Wind, GOES, LANL.IUGONETTohoku UNIPRSTEL, Nagoya UHida Obs., Kyoto URISH, Kyoto UWDC, Kyoto USERC, Kyushu UAutomatic data download by http from data servers①③②Users can get and analyze various kinds of observation data without any concerns about data locations.2. Overview of the TDAS/UDAS software2.3 Characteristics of the TDAS software-3TDAS has many useful routines to visualize and analyze time series data.By using the TDAS software, everybody can easily1. Make several time-series plots of many kinds of observation data in different fields over a long period. 2. Change the vertical and horizontal axes of the plots.3. Calculate time derivative and low or high pass filtered data 4. Display dynamic spectra of solar radio waves and geomagnetic field pulsation）6. Plot the kerograms for aurora and optical image data7. Make time-height contour plots for three dimensional data （Neutral wind, echo power  of refractive waves etc.）2. Overview of the TDAS/UDAS software2.4 Characteristics of the TDAS software-4TDAS has the work of Graphical User Interface (GUI) for beginner IDL users. In the GUI mode, you can easily analyze and visualize various kinds of observation data with only the mouse clicks and key bode enter.GUI top window2. Overview of the TDAS/UDAS software2.5 Load procedures of the UDAS in beta version 1. Load procedures of observation data related to the ERG project:• erg_load_gmag_mm210  ; 210°geomagnetic data （Nagoya, Kyushu, NICT, Tohoku）• erg_load_gmag_nipr ; geomagnetic data at Syowa , Ice Land （NIPR）2. Load procesures of the observation data provided from the IUGONET project:• iug_load_blr_rish_txt ; BLR（RISH, Kyoto）• iug_load_ltr_rish_txt ; L-band LTR （ RISH, Kyoto ）• iug_load_ear ; Equatorial Atmosphere Radar (EAR) （RISH, Kyoto）• iug_load_gmag_serc ; MAGDAS geomagnetic data （Kyushu）• iug_load_gmag_wdc ; AE, Dst, Sym, Asym induces, geomagnetic data （WDC, Kyoto）• iug_load_iprt ; IPRT （Tohoku）• iug_load_mu ; Middle and Upper (MU) atmosphere radar （RISH, Kyoto）• iug_load_meteor_rish ; Meteor wind radar（RISH, Kyoto）• iug_load_mf_rish ; MF radar （RISH, Kyoto）• iug_load_gmag_mm210 ; Elias of erg_load_gmag_mm210• iug_load_gmag_nipr ; Elias of erg_load_gmag_nipr3. Load procedures of other data provided in the future ：• erg_load_sdfit ; SuperDARN （Nagoya, NIPR, NICT）• erg_load_eiscat ; EISCAT（Nagogya, NIPR）3. RISH database of MW and MF radarsMF radar Pontianak (1995- ）★★★★MF radarPameungpeuk (2004-)Regional network in Indonesia (1992- ) Meteor wind radar(Jakarta, Kototabang) MF radar(Pontianak,           Pameungpeuk)Meteor radarJakarta (1992-1999)3.1 Regional network in Indonesia (MW and MF radars)Meteor radarKototabang (2002-)3. RISH database of MW and MF radars3.2 MF and MW radar database1．Meteor wind radar (Kototabang, Serpong)http://database.rish.kyoto-u.ac.jp/arch/iugonet/data/mwr/Numerical data：Serpong (1992/10-1999/08)Kototabang (2002/11～present)(1) Wind data ⇒Format: text, NetCDFTime resolution: 1 hour(2) Original data (Kototabang) ⇒Format: text (mp****.mpd)The original data include the radial Doppler velocity,  azimuth and zenith angles etc. for each meteor event.※Users can get these numerical data from the metadata search site. However, they can download and analyze only the wind data using the UDAS software. 3. RISH database of MW and MF radars3.2 MF and MW radar database2. MF radar (Pameungpeuk)http://database.rish.kyoto-u.ac.jp/arch/iugonet/data/mf/Numerical data： Pameungpeuk (2004/03～present)Format: Binary, NetCDFTime resolution：104 seconds※The NetCDF data include only the three components of wind data in  the MLT region (52-122 km), while the binary data include all the data set of radar status and wind observation data.※Users can get these numerical data from the metadata search system and UDAS software. Users can easily analyze and visualize the wind data obtained at the Pameungpeuk site.3. RISH database of MW and MF radars3.3 MF and MW radar database HomepageUsers can directly get the wind observation data of the MF and MW radars..Because the MW radar data include the wind data in the text format, users can analysis other softwares; for example excel, delta-gragh etc.4. Demonstration of the UDAS software4.1 Analysis and plot of the observation data in the CUI mode> timespan, ‘2003-10-01’, 31, /day (One month from October 1, 2003)> iug_load_meteor_rish_nc, site = ‘ktb’, parameter = ‘h2t60min00’> tplot_names （Confirmation of the tplot variable names）> tplot, ‘tplot variable names’⇒A time series plot is displayed in the other window. ※Multiple plots ： > tplot, [‘tplot1’, ‘tplot2’,…]> ylim, ‘tplot variable names’, (lower), (upper) [Height range]> zlim, ‘tplot variable names’, (lower), (upper) [color bar range]> tlimit, ‘tplot variable names’,  ‘2003-10-01’, ‘2003-10-15’ [time range](ex.) Plot of the wind data obtained from the Kototabang MWRStart of IDL⇒enter ”thm_init” on the IDL command line4. Demonstration of the UDAS software4.1 Analysis and plot of the observation data in the CUI modeOutput of time series plots of several parameters of the wind data 4. Demonstration of the UDAS software4.2 Examples of time series plots made in the CUI modeHokkaido SuperDARN radarGemag. (NIPR) SyowaIce landSolar radio waves by IPRT4. Demonstration of the UDAS software4.3 An example of the upper atmosphere research2006/12/14-16 Gemag. (KAK)MF radar  (PAM)EAR (trop.)SuperDARN (HOK)E-W windN-S windE-W windN-S windE-W plasma driftStorm commencementN-S plasma driftGeomagnetic storm00:00 08:00 16:00 00:00 16:0008:00 00:004. Demonstration of the UDAS software4.4 Analysis and plot of the observation data in the GUI mode•Even the IDL beginners can easily analyze and make time series plots of various kinds of observation data in the GUI mode.•The IUGONET project will provide the complied GUI execute file for the users with no IDL license in the future. ※Users can use this execute file with the IDL-Virtual Machinewhich is freely provided from the ITT.※However, there are several modifications of the TDAS-GUI in order to execute this file on the IDL-VM with no error. 3. Demonstration of the UDAS softwareData load window Select of instruments and geomagnetic indicesIn the present version, you can select 10 items.1．Geomagnetic indices2．Fluxgate magnetometer3． EAR(Troposphere/Ionosphere)4．MF radar5．Meteor wind radar6．MU radar(Troposphere)7．BLR8．LTR9. IPRT10. SuperDARNSelect of time rage of data load and plot.3.4 Analysis and plot of the observation data in the GUI mode3. Demonstration of the UDAS softwareMF radar (RISH)Lists of loaded dataMWR (RISH)Select of data type, observation site and parametersGeomag. Index (WDC)Gemag. KAK (WDC)Data load window3.4 Analysis and plot of the observation data in the GUI mode4. Demonstration of the UDAS softwareIf you try to load your selected data, acknowledgement is displayed on the other window.Select of ‘OK’：Finish the data loadingSelect of ‘Cancel’：Cancel the data loading.4.4 Analysis and plot of the observation data in the GUI modeAcknowledgement window3. Demonstration of the UDAS software3.4 Analysis and plot of the observation data in the GUI modePlot and layout option windowMake a time series plot (line) Make a time series plot (contour) Lists of plot data3. Demonstration of the UDAS software3.4 Analysis and plot of the observation data in the GUI modeGUI top window including height-time contour plotsE-W wind velocity (MF radar)N-S wind velocity (MF radar)E-W wind velocity (MW radar)N-S wind velocity (MW  radar)E-W wind velocity (BLR)Users can easily make time series contour and line plots for various kinds of observation data and change the vertical and horizontal scales with only the mouse click.In this GUI mode, users  can perform several simple data analyses of the loaded data; for example, average, time derivative, FFT, wavelet etc.5. Summary and future plan5.1 Summary and future plan of the UDAS softwareWe have developed the metadata database and integrated analysis software for ground observation data of the upper atmosphere in our IUGONET project.We develop the integrated analysis software which depends on the observation data of each institute, on the basis of the TDAS library written by the IDL language.The analysis software will be open for everybody who studies the Earth’s atmosphere after may this year.The IUGONET project will provide the complied GUI execute file (IDL save file) for the users with no IDL license in the future. We have started the cross-cutting research using various kinds of observation data provided from the IUGONET project. Our goal is to clarify the long-term variation of the upper atmosphere.  5. Summary and future plan5.2 Future plan of development of the UDAS softwareFMT photosphere pictureTwo-dimensinal plot tool of SuperDARN radar dataThe UDAS beta version does not include load procedures and plot tools of two-dimension data. We will develop the load and plot tools of two-dimension data (Sun, SuperDARN, Aurora) and open them for everybody as soon as possible next fiscal year. 

Development of integrated analysis software of observation data in the upper atmosphere

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Development of integrated analysis software of observation data in the upper atmosphere

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