Idl 8.5.1

2021年9月7日
Download here: http://gg.gg/vx9lx
*Idl 8 5 License
*Idl 8.4
*Idl 8.5
Clients running with recent run-time environments (e.g., Java 1.8.0102, IDL 8.5.1, etc. Or newer) will likely not have a problem using HTTPS. Clients using an older run-time may have to update their environment with newer Certificate Authority (CA) root certificates. Itt Idl 8.5 Envi 5.3 Crack Serial Keygen ※ Download: Envi idl crack - envi idl crack. If you have an IDL license, you can download the SPEDAS 3.2 release, which. SPEDAS 3.2, Windows 64bit executable with IDL 8.5.1, CDF 3.7.1. Files in the ’Program Files Exelis IDL84 bin bin.x8664’ folder (this folder.Idl 8 5 License2017-05-28 23:19:09 UTC Hi guys,I installed IDL 8.5.1 successfully on my MacOS Sierra 10.12.2 following the instructions fromhttp://www.harrisgeospatial.com/Support/Forums/tabid/2342/aft/4715/Default.aspxHowever, when I tried to set up the IDL-python bridge, I run into an issue (I’m using python 2.7, the preinstalled version on my mac, not Anaconda). When I ran:np = Python.Import(’numpy’)I got the error message:% DLM_LOAD: Error loading sharable executable.Symbol: IDL_Load, File = /Applications/exelis/idl85/bin/bin.darwin.x86_64/idl_python27.sodlopen(/Applications/exelis/idl85/bin/bin.darwin.x86_64/idl_python27.so, 1): Library not loaded: libpython2.7.dylibReferenced from: /Applications/exelis/idl85/bin/bin.darwin.x86_64/idl_python27.soReason: image not foundI searched the web and followed one post by Chris Torrence (http://stackoverflow.com/questions/38468764/idl-python-bridge-fails-due-to-sip-on-osx-el-capitan) to set up the path, but still got the same error. Here are the steps I did on my mac:First, set up the paths:export PATH /System/Library/Frameworks/Python.framework/Versions/2.7/bin:${PATH}export PYTHONHOME /System/Library/Frameworks/Python.framework/Versions/2.7export PYTHONPATH /Users/username/Applications/exelis/idl/bin/bin.darwin.x86_64export PYTHONPATH ${PYTHONPATH}:/Users/username/Applications/exelis/idl85/lib/bridgesThen, for the IDL-to-Python bridge, run the following commands:cd Applications/exelis/idl85/bin/bin.darwin.x86_64/sudo install_name_tool -change libpython2.7.dylib /System/Library/Frameworks/Python.framework/Versions/Current/lib/libpython2.7.dylib pythonidl27.soFor the Python-to-IDL bridge (some of these are duplicated from above):cd Applications/exelis/idl85/bin/bin.darwin.x86_64/sudo install_name_tool -change libidl.8.5.dylib @loader_path/libidl.8.5.dylib pythonidl27.sosudo install_name_tool -change libidl_ips.8.5.dylib @loader_path/libidl_ips.8.5.dylib pythonidl27.sosudo install_name_tool -change libpython2.7.dylib /System/Library/Frameworks/Python.framework/Versions/Current/lib/libpython2.7.dylib pythonidl27.soAt this point, DYLD_LIBRARY_PATH is still needed in the .login to specify IDL’s bin directory. To eliminate that, the following updates can be made to tell various libraries where to find their dependencies:sudo install_name_tool -change libMesaGL6_2.dylib @loader_path/libMesaGL6_2.dylib libidl.8.5.dylibsudo install_name_tool -change libMesaGLU6_2.dylib @loader_path/libMesaGLU6_2.dylib libidl.8.5.dylibsudo install_name_tool -change libOSMesa6_2.dylib @loader_path/libOSMesa6_2.dylib libidl.8.5.dylibsudo install_name_tool -change libXm.3.0.2.dylib @loader_path/libXm.3.0.2.dylib libidl.8.5.dylibsudo install_name_tool -change libMesaGL6_2.dylib @loader_path/libMesaGL6_2.dylib libMesaGLU6_2.dylibsudo install_name_tool -change libMesaGL6_2.dylib @loader_path/libMesaGL6_2.dylib libOSMesa6_2.dylibsudo install_name_tool -change libidl.8.5.dylib @loader_path/libidl.8.5.dylib libidl_ips.8.5.dylibAfter these settings, when I try to import python modules in IDL, the error message says Library not loaded: libpython2.7.dylib... Can anyone help me on this?Cheers,HuazengNews and Announcements + REPORTS+ STAFF+ SCIENCE ENABLED+ DATA SERVICE USAGE+ FEEDBACK/SUPPORT[April 2021]: The Parker Solar Probe (PSP) data have been extended to December 2020 - February 2021 in the SPDF archive and CDAWeb, and include Encounter 6 and the rest of Orbit 6. Most of the ISOIS datasets include new variables. This release adds a new ISOIS ephemeris dataset, a new SWEAP alpha particle distribution dataset, and reprocessed Digital Fields Board (DFB) cross spectra and subset of FIELDS MAG data. [November 18, 2020]: The Parker Solar Probe (PSP) data has been extended through August 2020, for most data sets, and includes encounter 5 and the remainder of orbit 5. The new data files were added to the CDAWeb system and to the SPDF PSP archive.[November 11, 2020]: Solar-Orbiter data: The insitu and ephemeris data from the Solar Orbiter mission are available at the SPDF Solar Orbiter archive. The Level 2 and above of science data as well as the low latency data are served at CDAWeb. All the data are mirrored from the ESA Solar Orbiter Archive.p>[September 2020]: The Parker Solar Probe (PSP) FIELDS and SWEAP data has been extended through April 2020, for most data sets. The new data files were added to the CDAWeb system and to the SPDF PSP archive.[August 2020]: GOLD L2 data is coming into the archive more frequently. See the data and the release notes[June 2020]: The Aeronomy of Ice in the Mesosphere (AIM) Cloud Imaging and Particle Size (CIPS) data products are available in the archive. Access the data and the documentation. The Polar Mesospheric Cloud (PMC) data are organized by hemisphere season each year, and the Rayleigh Albedo Anomaly (RAA) data are by month.[April 15, 2020]: Parker Solar Probe (PSP) data has been updated to January 14, 2020 (the start of the 4th orbit around the Sun). New data files have been added to the CDAWeb system and to the SPDF PSP archive. On February 10, 2020: the PSP data included the 3rd orbit about the Sun. [January 2020]: GOLD L1C and L1D data are being released more regularly now, beyond 11/30/2019. This includes Channel A and B data, except for Channel B data for the period 12/15/2018-3/15/2019 which are currently only available by special request from the GOLD website. The Level-2 data for O2DEN, beyond 8/13/2019, is also being released. The GOLD Global-scale Observations of the Limb and Disk Release Notes and data, Revision 3.1 (Dec 8, 2019), are available at the SPDF archive.[November 22, 2019]: Parker Solar Probe (PSP) data is available in the archive and all data sets are in CDAWeb. [September 19, 2019]: GOLD L1C, L1D, and L2 data files (Channel A) have been replaced with a new version in the SPDF archive. L1C and L1D data were updated to include a flat-field correction (DAY, LIM, and OCC to version 02; NI1 to version 03). L1 data are available through 8/13/2019. L2 data products were updated based on the new L1 data. TDISK, TLIMB, O2DEN, and ON2 (v02) are available through 8/13/2019. The initial release of QEUV data (v01) is available through 1/31/2019.[August 1, 2019]: Change from FTP to FTPS As part of Federal policy to encrypt all network connections, FTP access to the SPDF and CDAWeb data archive was changed to TLS-encrypted FTPS on July 31, 2019. Browsers and traditional command line FTP will NO LONGER CONNECT with FTP, but HTTPS access remains. For more information and alternatives, see our FTPS Readme.[June 25, 2019] Robert McGuire, the head of the Space Physics Data Facility (SPDF) since 1992, has retired. He started as a National Academy of Sciences (NAS) Post-doctoral Fellow at NASA Goddard in 1976, served as the last Project Scientist for the IMP-8 mission until 2006 and was the last designated Principal Investigator of the IMP-8 Goddard Medium Energy (GME) (energetic particle) experiment. He was the Associate Director for Science Information Systems in the Heliophysics Science Division at Goddard.
He has been succeeded as Project Scientist for SPDF by Robert M. Candey with Lan Jian as Deputy.[June 25, 2019] GIFWALK update: The Canned plot visualizer interface has been updated to display MMS Quick Look Summary plots.[February 2017 (Updated July 2018)]: Space Physics Data Facility (SPDF) web sites changed to use HTTPS (TLS V1.1 & V1.2) instead of HTTP:Scientific data from many heliophysics missions are available at the Space Physics Data Facility (SPDF) through web pages or by using the Heliophysics Data Portal. This includes CDAWeb data browsing, SSCweb orbit displays and the OMNIWeb as well as the CDF software pages.
All of these SPDF web sites and web services have changed from HTTP to HTTPS to provide assurance that you are accessing the servers you expect and not imposter sites. This change has been planned for some time and is in keeping with the rest of the US Government. FTP data access is not affected at this time.
For most people, this will be transparent since current versions of browsers will redirect automatically to the HTTPS pages. However, this may be an important and immediate concern for developers and users of SPDF Web Services inside Java, IDL or other software packages, since most web service calls will BREAK until updated to specify HTTPS instead.
SPDF web services and some clients - that need to be changed to HTTPS:CDAS: https://cdaweb.gsfc.nasa.gov/WebServices/SSC: https://sscweb.gsfc.nasa.gov/WebServices/IDL CREADER: https://hpde.gsfc.nasa.gov/CDAWeb_to_IDL.htmlCalls to OMNIweb inside software packages: https://omniweb.gsfc.nasa.gov/Also SPDF web services from the SPEDAS IDL library: http://spedas.org/wiki/
Clients running with recent run-time environments (e.g., Java 1.8.0_102, IDL 8.5.1, etc. or newer) will likely not have a problem using HTTPS. Clients using an older run-time may have to update their environment with newer Certificate Authority (CA) root certificates. Additional information about accessing these web services over HTTPS is available at https://sscweb.gsfc.nasa.gov/WebServices/https.html
Any questions or comments concerning this release should be emailed to NASA-SPDF-Support@nasa.onmicrosoft.com.[October 2016]: CDF Version 3.6.3.1 Released:
Common Data Format (CDF) Version 3.6.3.1 is now available. This release contains a minor change to the earlier release of V3.6.3.0 and includes a new leap second added for 1/1/2017. Please read the change notes that describe the changes made in this release, as well as all previous releases. Updates for Perl, IDL, Matlab, and Java interfaces and the SKTeditor CDF editor are also available.[2016]: Revised Definition of the Sunspot Number Index:
Sunspot Number Index values 1963-2015 in OMNI have been updated to the revised Version 2 definition now used by the Royal Observatory of Belgium. The updated values are generally larger by factors 1.2-1.7 and can be compared in detail using OMNIWeb’s sunspot index comparison tool.[2014-Oct-14]:New CDF Version 3.6.0 Released:
The Space Physics Data Facility (SPDF) at NASA Goddard Space Flight Center has issued an important update to its Common Data Format (CDF) package of software APIs and tools. We strongly urge all CDF users to promptly upgrade their CDF software to this latest release (version 3.6) to better ensure the correct handling of times after the 2015 June 30 leap second. Updates for Perl, IDL, Matlab, and Java interfaces are also available. CDAWeb is currently receiving and also producing CDF 3.6 files.
Besides many minor software updates and fixes, this release includes an updated internal leap second table and now preserves (in the CDF file header) this latest leap second available when a CDF is written. This enables a warning when CDF_TIME_TT2000 times may have been computed with an out-of-date leap second table and thus may be incorrect. CDFconvert has additional options for sorting on a specified variable, resetting the blocking factor, updating the CDF header for the latest leap second, and adjusting CDF_TIME_TT2000 times written with an out-dated leap second table. For further details, see the CDF release notes.
The SPDF’s SKTEditor program was also upgraded for this new release and includes additional validation options.
We also encourage all to subscribe to the CDF Announcements email list to receive warnings of future leap seconds and other CDF issues. As always, please report any problems, issues or questions to NASA-SPDF-Support@nasa.onmicrosoft.com.
Michael Liu and Robert Candey[2014-Oct-14]:New CDF Version 3.5.0 Released:
NASA’s Space Physics Data Facility (SPDF) is pleased to announce the release of Version 3.5.0 of the CDF software. In addition to many minor software updates and fixes, the software now includes the open source version of zlib for doing gzip compression, new support for Visual Basic for Windows, additional C/Fortran functions and enhancements to the toolkit programs. For further details please read the CDF release notes.[2013-Aug-28]:Current MagED Data from GOES 13/14/15 Now Available in CDAWeb:
NOAA’s National Geophysical Data Center (NGDC) and NASA’s Space Physics Data Facility (SPDF) are pleased to announce a joint long-term effort to make a variety of appropriate current GOES and POES heliophysics data available through SPDF’s CDAWeb multi-mission data service. As the first of many data products we expect to eventually support, current GOES 13 and 15 1-minute and 5-minute electron flux data from the Energetic Particle Suite (EPS) Magnetospheric Energetic Detectors (MagEDs) are now available in CDAWeb including graphics, listings, superset/subsets in CDF, FTP/HTTP downloads, via CDAWeb web services calls and within IDL sessions using the SPDF’s Cdas library. GOES 14 MagED data for Oct-Nov 2012 (before this s/c was put in orbital storage) are also available.
CDAWeb access supplements the existing distribution of this data in CSV and netCDF format from the NGDC archival services. MagED data consist of electron fluxes 40 - 475 keV in 9 look directions, with data from GOES 13 from January 2011 through June 2013, data from GOES 15 from February 2011 to the present.[2013-Jun-11]:Data from NASA’s Van Allen Probes Now Available in CDAWeb:
With thanks and all credit to the dedicated work of the project and instrument teams, the Space Physics Data Facility is pleased to announce availability in CDAWeb of some 70 new Level-2 and Level-3 datasets from the Van Allen Probes spacecraft, previously known as the Radiation Belt StormProbes or RBSP. While additional datasets will become available over the next few months, this data collection fully spans the range of measurements from particles-plasma (RBSPICE, ECT) through magnetic-electric fields and waves (EMFISIS, EFW) with data generally current to within 60 days or less. The research community is referred to the project pages and particularly to the information and links on the science Gateway page for more complete descriptions of the spacecraft and instruments, the correct meaning and appropriate use of Van Allen data, space weather and summary plots of various kinds, and a range of other highlyuseful and more specialized data services at the instrument sites. The full set of data and services for the Van Allen Probes will be the focus of a special session on Tuesday afternoon June 18th at the GEM meeting in Snowmass, Colorado.
The project, instrument teams and SPDF hope that including these already-public data in the CDAWeb database will make access and use of this data (e.g. plots, listings, supersets and subsets, direct downloads by FTP and HTTP, links to key capabilities at the instrument team sites) more convenient for the science community. Having this range of data in CDAWeb makes comparison of data among instruments and spacecraft much easier, as well as comparisons and analysis of these data versus current data from other missions such as THEMIS, TWINS, Cluster, ACE, Wind and the >120 ground magnetometer stations also in CDAWeb. All these data are also available through the SPDF web- services interfaces and e.g. our spdfcdawebchooser routine that allows direct selection and ingest of data from CDAWeb into an IDL session (cf.SPDF’s Cdas library)., Van Allen Probes orbits are fully supported in our SSCWeb and 4-D Orbit Viewer services.[2012-Sep-24]:Relocation of Directories and Files Served by FTP by SPDF and NSSDC:
On September 24 and 25, the Space Physics Data Facility (SPDF) renamed and restructured its FTP and HTTP accessible directories. This newly unified structure merges CDAWeb files already served by SPDF with legacy heliophysics data holdings that have been served by the National Space Science Data Center (NSSDC) on nssdcftp.gsfc.nasa.gov. The responsibility for the final archiving of heliophysics has been transferred from NSSDC to SPDF (for non-solar instruments) and to Solar Data Analysis Center (SDAC) (for solar instruments). SPDF will also serve legacy solar instrument data previously served by NSSDC on at least an interim basis.
All heliophysics data and other files previously accessible separately from NSSDCftp or CDAWeb are accessible from any of the following links:FTP SPDF,SPDF,FTP CDAWeb,CDAWeb.
Other SPDF services are unchanged.
Any databases or services that point to specific server and directory locations on CDAWeb and NSSDCftp will need to update their records to these new locations. A list of directories as now moved (current and new locations) is posted here.
Changes to CDAWeb data directories are listed first and directories moved from NSSDCftp are listed second. Data now on NSSDCftp may continue to be available on NSSDCftp for a limited time after this official move.
SPDF regrets that this level of re-naming and re-structuring of our data holdings cannot be made fully transparent to users. Please report any problems and discrepancies to us atNASA-SPDF-Support@nasa.onmicrosoft.com.[2012-Jun-20]:Let’s Not Lose Our Data :
Along with the Solar Data Analysis Center (SDAC), the Space Physics Data Facility (SPDF) is charged with ensuring the long-term preservation and ongoing availability of important data from NASA heliophysics investigations, with interest as well in other data relevant to current NASA heliophysics science objectives.
SPDF is concerned that important data from older missions (past and current) are at increasing risk of being lost as projects and their funding expire, and as the scientists responsible for the data move to new missions, change responsibilities or retire. So I ask that you please carefully consider the status of any data you may now hold:
*Does it have potential long-term value to our research community?
*Is it now held on aging media or systems?
*Is it held where there may not be ongoing funding to ensure continued preservation and access?
Everyone with a direct role in collecting or analyzing space data knows the investment in time and resources represented in such data. For the data you hold and work with, you know the important science in your data that may still remain unexploited. Very high time resolution measurements and particle distribution functions are among the kinds of data that could be of special interest.
If you have or know of existing heliophysics data that might be a concern, please contact me as the Project Scien

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