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  3. باربری تهران

    باربری تهران باربری تهرانبا سالها سابقه و تجربه درخشان در حمل اثاثیه در تهران اماده ارائه خدمات به همشریان عزیز را دارا است.هرساله با نزدیک شدن به موقع اثاث کشی مستاجر ها و کسانی که قصد دارند خانه خود را به مقصد خانه جدید ترک کنند با یک دغدغه با نام اثاث کشی روبرو میشوند:که شامل جمع اوری.جابجای.چیدمان و بسته بندی می باشد. اتوبار تهران بار متخصص در امر باربری حمل اثاث منزل.ادارات.شرکت ها و ارگان های دولتی.مبلمان…با بهرگیری از بهترین سرویس دهی باربری تهران پیشرو در کلیه امور خدماتی در گروه باربری در تهران اماده سرویس دهی ، وانت . خاور . نیسان و شهرستان ، و متخصص در باز و بسته کردن درب انواع یخچال ساید و معمولی ،تخت های بغل باز شو و تردمیل ،با پرسنل خوب و ماهر با سابقه کاری در تهران آماده خدمت رسانی است باربری تهران با توجه به تغییرات روز افزون امکانات و تجهیزات باربری همواره سخت در تلاش است تا خود را با این امکانات مجهز کرده و بهترین خدمت گذاری را به شما همشهریان گرامی ارائه دهد. 02144303890
  4. Last week
  5. ODE - Mars Odyssey Release 62 Data Loaded into ODE

    January 18th, 2018 --Loaded NS and HEND raw and derived data into ODE through June 30th, 2017 See https://wufs.wustl.edu/ode/odeholdings/Mars_holdings.html.
  6. Odyssey Release 62

    Mars Odyssey Release 62 includes new raw data (EDR) , Derived Neutron Data (DND) and Derived HEND Data (DHD) products covering the period April1 through June 30, 2017. Averaged Neutron Data (AND) and Averaged HEND Data (AHD) products cover the period March 10, 2017 to July 8, 2017, Ls 330 in year 08 to Ls 15 in year 09. The data are online at the PDS Geosciences Node at http://pds-geoscienc...dyssey/grs.html.
  7. Earlier
  8. January 12th, 2018 –Interim Releases of MRO SHARAD EDR data loaded into ODE. Updated SHARAD EDR products from December 6th, 2006 to February 21st, 2015 (orbits through -40185) Interim Release. January 12, 2018. ---------------------------------- This release includes a redelivery of select EDR datasets due to errors in the selection of corresponding raw data files. The affected IDs are: edr2689301 edr2695502 edr2689501 edr2695801 edr2690401 edr2698501 edr2692001 edr2717901 edr2692401 edr2720601 edr2692402 edr3325001 edr2693301 edr3334301 edr2695201 edr3486101 edr2695501 Interim Release. January 4, 2018. --------------------------------- Two errors were discovered in the SHARAD Auxiliary Data Files for releases 23 through 34. The value of Orbit Number and the sign of Spacecraft Radial Velocity were incorrect. This release corrects all the errors in the affected observations. See https://wufs.wustl.edu/ode/odeholdings/Mars_holdings.html See ERRATA.TXT (http://pds-geosciences.wustl.edu/mro/mro-m-sharad-3-edr-v1/mrosh_0003/errata.txt) for more details.
  9. January 12, 2018 – MRO HiRISE Updates - MRO HiRISE EDR, RDR, DTM and Anaglyph data products released through December 1, 2017 (Orbit 53,199) See https://wufs.wustl.edu/ode/odeholdings/Mars_holdings.html
  10. January 11th, 2018 – The third release of Earth-based Venus radar data from Bruce Campbell loaded into ODE. This release contains data collected from August 10 - August 16, 2015 and March 21 - March 27, 2017. See below links for more details http://pds-geosciences.wustl.edu/missions/venus_radar/index.htm https://wufs.wustl.edu/ode/odeholdings/Venus_holdings.html
  11. A new batch of Earth-based Venus radar data has been released on the PDS Geosciences Node web site at http://pds-geoscienc...radar/index.htm. This release contains data collected from August 10 - August 16, 2015 and March 21 - March 27, 2017. This data set contains Earth-based, polarimetric radar image data for Venus collected from 1988 onwards, using the Arecibo Observatory 12.6-cm (2380 MHz) transmitter in Puerto Rico and receivers at either the Arecibo Observatory or the Green Bank Telescope in West Virginia. The data were provided by Bruce Campbell of the Smithsonian Institution's Center for Earth and Planetary Studies and archived by the PDS Geosciences Node.
  12. ODE has recently released a new ODE cart request download page. This is a new option for accessing a requested ODE cart request. A link to the page is provided in the order fulfillment email that a user receives after their cart request is ready for download. The new ODE cart request download page supports multiple download methods and offers faster options for users to retrieve requested ODS files. The ODE cart request download page contains a single click link to download the entire user cart request using the Aspera Connect web browser plug-in. This option provides a convenient and fast download method for most users. The Aspera Connect browser plug-in employs the FASP data transfer technology to better utilize the user’s available bandwidth. HTTP and FTP links are provided on the page for users who prefer to download the files through a client application, a different web browser plug-in, a local script, or directly through the web browser. Additionally, the page supports browsing and downloading specific directories and files of the cart request through the Aspera Connect web browser plug-in or using direct HTTP links. Multiple files can be downloaded simultaneously through this page. Try the new page the next time you request PDS products through the ODE cart!
  13. ODE has recently added a new option to download all of a PDS product's files through a single click. The new option is available from the product detail page of PDS products hosted by the PDS Geosciences Node. This option uses the Aspera Connect browser plug-in. Aspera technology more fully utilizes one's available bandwidth than traditional TCP connections, such as HTTP and FTP, which will improve the speed the file download speed. Give the new feature a try and let us know how it works for you. Example page with the option: http://ode.rsl.wustl.edu/mars/indexproductpage.aspx?product_id=FRT0000B278_07_IF164S_TRR3&product_idGeo=17880484 Help page further describing the feature and installation of the Aspera Connect browser plug-in: http://ode.rsl.wustl.edu/mars/pagehelp/quickstartguide/index.html?product_detail_page.htm#aspera
  14. January 5th, 2018 - Mar Odyssey Release 62 THEMIS Data Updates Updated THEMIS standard data products (IREDR, IRRDR, IRBTR, VISEDR, VISRDR and VISABR data) from February 19th, 2002 to June 9th, 2017 Updated THEMIS geometry data products (IRGEO2, IRPBT2, VGEO2, and VISALB data) from September 28th, 2013 to June 9th, 2017 Release 62 of NS and HEND data is delayed. The data would be available by January 15, 2018. See https://wufs.wustl.edu/ode/odeholdings/Mars_holdings.html.
  15. ODE - LRO Release 32 Loaded into ODE

    Jan 2, 2018 Updated Diviner RDR query tool database from July 5th, 2009 to September 15th, 2017.
  16. MER Release 54

    Data from Release 54 of the Mars Exploration Rover mission is now online at the PDS Geosciences Node. This release includes APXS, Atmospheric Opacity, MI, Navcam, Pancam, RAT, and Rover Motion Counter data from sols 4681 through 4770 for the Opportunity rover.
  17. December 19th, 2017 - LRO Release 32 has been loaded into ODE. Updated LOLA EDR products from June 18th, 2009 to September 20th, 2017 Updated LOLA RDR products from July 13th, 2009 to September 20th, 2017 Updated LAMP EDR and RDR products from July 6th, 2009 to September 15th, 2017 Updated LEND EDR_SCI, EDR_HK, RDR_RSCI, and RDR_CHK products from June 18th, 2009 to September 14th, 2017 Updated LEND RDR_DLD and RDR_DLX products from June 27th, 2009 to June 14th, 2017 Updated Diviner EDR and RDR products from July 5th, 2009 to September 16th, 2017 Updated Diviner GDR products from July 5th, 2009 to October 23rd, 2016 Updated LROC EDR, CDR and RDR products from June 30th, 2009 to September 15th, 2017 Updated LOLA RDR query tool database from July 13th, 2009 to September 20th, 2017 In Progress Diviner RDR query tool database from July 5th, 2009 to September 15th, 2017. A few LOLA GDR count gridded products have been revised; see ERRATA.TXT for details. Please see ODE Lunar Holdings - https://wufs.wustl.edu/ode/odeholdings/Moon_holdings.html
  18. Use of uncertainties in gravity model

    Alvaro, I took your question to Frank Lemoine on the MRO gravity team. His reply is below. Susie Slavney From Frank: "The uncertainties that are provided with a gravity model are derived from the diagonal of the covariance matrix of the spherical harmonic solution. They are representation of the coefficient error, but do not account for the correlations between the coefficients in the least squares solution. In order to obtain another realization of the gravity field solution that is perturbed according to the error information in the covariance, it is necessary to create clones, as discussed in this document (developed as part of the work on the GRAIL mission). http://pds-geosciences.wustl.edu/grail/grail-l-lgrs-5-rdr-v1/grail_1001/extras/clones/clone_description.pdf For Mars, the GSFC team has created clones of the GMM-3 gravity model which might be suitable for the user. This model is described in the paper by Antonio Genova et al. (Icarus, 2016). The clones of GMM-3 are available at the following URL. http://pds-geosciences.wustl.edu/mro/mro-m-rss-5-sdp-v1/mrors_1xxx/extras/clones/ The GMM-3 model is available at the following URL. http://pds-geosciences.wustl.edu/mro/mro-m-rss-5-sdp-v1/mrors_1xxx/data/shadr/gmm3_120_sha.tab The descriptive Label for the model is available at this URL. http://pds-geosciences.wustl.edu/mro/mro-m-rss-5-sdp-v1/mrors_1xxx/data/shadr/gmm3_120_sha.lbl If the user wishes to create clones for the JPL gravity model, they can either ask Alex Konopliv at JPL, or download the error covariance (the SHBDR file), and follow the procedure in the above pdf document to manufacture their own gravity field clones. Sincerely, Frank Lemoine NASA Goddard Space Flight Center "
  19. Good morning I was looknig at the gravitational data provided in JGMRO_110C_SHA.TAB and I could not understand how to use the uncertainties provided. I see that for example the third column of the first line provides a value of 1.9E-05 and the description of this number is "For a gravity field model the uncertainty in the gravitational constant GM in kilometers cubed per seconds squared for the planet" I wanted to generate a "perturbed" gravity field based on this uncertainty. How would you recommend to do it? Shall I assume a uniform distribution and compute the Real_GM = Nominal_GM + uniform(-1,1)*uncertainty Or do you recomend using a gaussian distribution using the uncertainty as 1-sigma value? In a similar way, the file also provides uncertainties for the coefficients Cmn and Smn. How shall understand this uncertainties if I want to create a perturbed (non-nominal) gravity field using all the coefficients and uncertainties provided in the file? Should I use a similar formulation of the one presented above? Many thanks in advance Kind regards, Alvaro
  20. CAT 7.3.1 in ENVI 5.4

    Hi Al, I am ready to help. The problem to me seems an IDL_PATH issue. Would you please verify the following path in the idl.pref file (in default installation, it locates C:\Program Files\Harris\ENVI54\IDL86\resource\pref folder)? IDL_PATH: + C:\Programmi\CAT_ENVI;<IDL_DEFAULT> If there is no such statement in this file, would you please add it? Let's me know if you do see this path. Thanks, Feng Friday at 10:31 AM Edit Report Al Emran Hi Feng, Thank you for the reply. Yes, I have solved the problem. Thanks, Emran Sunday at 04:16 PM 0 Report
  21. December 3rd, 2017 - MRO Release 43 Loaded into ODE. - Updated MRO CRISM EDR and CDR products from September 27th, 2006 to August 9th, 2017 - Updated MRO CRISM DDR products from September 27th, 2006 to July 15th, 2017 - Updated MRO CRISM TRDR products from September 27th, 2006 to July 15th, 2017 - Updated MRO raw gravity data products released through July 26th, 2017 - Updated SHARAD Radargram data products released through May 12th, 2017 (orbits through 50596). - Updated MRO MCS EDR, RDR and DDR products from September 15th, 2006 to July 31st, 2017 - Updated MRO CTX EDR products from August 30th, 2006 to May 31st, 2017 - Updated MRO HiRISE EDR, RDR, anaglyph and DTM products released through October 31st (Orbit 52799), 2017 Please see ODE Mars Holdings – https://wufs.wustl.edu/ode/odeholdings/Mars_holdings.html
  22. Hi Al,

    I am ready to help. The problem to me seems an IDL_PATH issue. Would you please verify the following path in the idl.pref file (in default installation, it locates C:\Program Files\Harris\ENVI54\IDL86\resource\pref folder)?

    IDL_PATH: + C:\Programmi\CAT_ENVI;<IDL_DEFAULT>

    If there is no such statement in this file, would you please add it? Let's me know if you do see this path.

     

    Thanks,

     

    Feng

     

    1. Al Emran

      Al Emran

      Hi Feng,

      Thank you for the reply. Yes, I have solved the problem.

      Thanks,

      Emran

  23. CAT 7.3.1 in ENVI 5.4

    Hello, I installed CAT 7.3.1. in ENVI 5.4 as per the instruction. ENVI shows CAT tool neither in menubar nor under Display. An extension toolbox has created named ''cat_menu'' (see attachment). But, this icon doesn't work also! How can I fix this? Thank you,
  24. Overlay M3 and RELAB spectra

    Attached are some slides showing how I used ENVI to ingest M3 lunar data and lab data, resample the lab data to the M3 wavelengths, and overplot the two data sets. Ray Arvidson PDS Geosciences Node Manager spectral_resampling.pdf
  25. November 11th, 2017 - THEMIS IR-reprocessed data from releases 0048, 0049, and 0050 (orbits 52300-55599) have been loaded into ODE. Please see ODE Mars Holdings – https://wufs.wustl.edu/ode/odeholdings/Mars_holdings.html
  26. Mars elevation data: longtitude, lattitude, elevation.

    I asked the ODE developer if she could suggest a way to do this. Here's her answer. She reads this forum too. Hi Susie, Below link shows an example on how to read those MEGDR products with Matlab. The user could modify the code a little bit to output a table with lat, lon, and height. https://www.mathworks.com/matlabcentral/fileexchange/13444-using-data-from-mola?focused=6780621&tab=example&requestedDomain=www.mathworks.com Another way is to convert the PDS IMG to ERDAS IMG in ArcGIS. Then use ERDAS to convert the ERDAS IMG to an ASCII table with lat, lon, and height. Both Matlab and ERDAS are commercial software. Otherwise, the user needs to write his own program to read the PDS IMG data. The label includes everything that the user needs to know to read the data file. Please let me know if the user needs further help. Thanks, June
  27. Overlay M3 and RELAB spectra

    Here to help. I am not sure why you have a screen shot of a vertical profile, which suggests to me you opened the spectral library as an image. To examine the spectral library data you need to open the file as a spectral library, not as an image. Did you open it as a spectral library, and could you display spectra? If you did this and can display spectra, resampled to M3 bandpasses, you should be able to overlay spectra from an M3 cube pixel with the lab spectra. Let me know what you did and I can help more if the instructions above are not enough. Worst case is for me to try what you wanted to do with the exact data sets you used. Ray Arvidson
  28. The query tool you mentioned is for PEDRs, I'd like to look at the globally gridded MEGDR products. When I use the ODE data product search (as suggested at the top of the PEDR Query Tool 2 page), I can bring up a file, for example MEGT90N180GB.IMG, however, the PDS product files and Derived files do not include a simple text table (lat, lon, elevation), it only includes more images and some shapefiles. What is the easiest way to convert the MEGDR products to a simple text table?
  29. Mars elevation data: longtitude, lattitude, elevation.

    The MOLA PEDR Query Tool I mentioned before will allow you to create output as an ASCII text file.
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