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<p>The SPEDAS development team is pleased to announce the release of SPEDAS 3.2! </p>
<p>SPEDAS 3.2 includes numerous updates and enhancements to the
command-line tplot plotting and analysis tools, as well as the Graphical
User Interface (GUI). The CDF support code has been updated with
improved functionality and performance under different IDL releases and
CDF library versions. The SPEDAS tools for interacting with the CDAWeb
archive, HAPI servers, and Autoplot have also been improved. This
release also includes the latest available versions of the MMS, ERG
(Arase), IUGONET, and Akebono plugins from their respective developers,
along with incremental updates to the support for THEMIS, GOES, WIND,
and other missions.</p>
<p>SPEDAS 3.2 also includes command-line tools (under the projects/SPP
directory) for working with Parker Solar Probe data, which has recently
been publicly released</p>
<p>For a more detailed list of new features, enhancements, and bug fixes since SPEDAS 3.1, please see the release notes, at <a href="http://spedas.org/downloads/SPEDAS_3_2_release_notes.pdf">http://spedas.org/downloads/SPEDAS_3_2_release_notes.pdf</a></p>
<p>As usual, SPEDAS 3.2 is available as a source code zip file (suitable
for users with full IDL licenses). For users without IDL licenses, we
have also released the SPEDAS 3.2 “virtual machine” executables for
Linux, Mac, and Windows. SPEDAS 3.2 downloads, installation
instructions, and platform-specific installation notes are available via
the <a href="http://spedas.org/wiki/index.php?title=Downloads_and_Installation">SPEDAS wiki Downloads and Installation page</a> .</p>
<p>Please email questions, bug reports, help requests, and enhancement suggestions to <a href="mailto:SPEDAS_Science_Support@ssl.berkeley.edu" rel="noreferrer noopener" target="_blank">SPEDAS_Science_Support@ssl.berkeley.edu</a></p><p>The <span class="gmail-il">SPEDAS</span> software development has been supported by NASA contracts
NAS5-02099 (THEMIS mission), NNG17PZ01C (<span class="gmail-il">SPEDAS</span> general development),
and NNG04EB99C (MMS sub-contract). We would also like to thank the many
software developers and <span class="gmail-il">SPEDAS</span> users who have supported the development
effort by contributing code, reporting problems, and suggesting
enhancements.
</p><p>Cheers,</p><p>Jim Lewis, on behalf of the SPEDAS development team<br></p>
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