Ism V6.2 Download
Yolette Langevin
We use Hyper-V, running on Windows Server 2012 R2. Creating the VM using the ERA_Appliance_v6.5.31.0.vhd file works fine. Pulling the database across from the old appliance to the new, and restoring it seems to work fine. However, failure occurs after having set up the new appliance for the first time, from its web console. After this, the new appliance restarts and gives the error "First time appliance configuration failed".
Migration via this method to v6.5.31.0 is listed as being supported on all previous 6.x versions of the VA, but it's not working for me. Backing up the old database from the v6.2.200.0 VM isn't listed as an option in its VM management mode console, unlike newer versions, else I'd try setting up the new server afresh and then restore the old database to it after it is completely up and running.
On restarting the new VM after the initial web configuration, and being given the "First time appliance configuration failed." error, I thought I'd log in to the Webmin web console for further investigation (enter the management mode of the VM, and choose "Enable/Disable Webmin interface" to toggle this on/off - by default it was disabled). Once in Webmin, there was an entry under Servers for ESET Remote Administrator, but this was blank, probably as to be expected. The Webmin Dashboard was flagging up that there were package updates available (290 of them), so I thought it was worth a try. I let these package updates download and install, and restarted the VM.
After this, I logged back on to the web console for VA configuration (hxxp://help.eset.com/era_deploy_va/65/en-US/index.html?config_va.htm), choosing "ESET Remote Administrator Server Appliance" again, for the initial set up. I only entered something in the password field, as shown below, leaving all the network setting fields blank (as I have done previously). "Submit" was clicked, the VM restarted, and the VM console then loaded without the "First time appliance configuration failed." error, showing "Server version: 6.5.417.0, Agent version: 6.5.417.0, Rogue Detection Sensor version: 1.0.1079.0). Huzzah!
On logging in to the new ERA web console (port 8443), the old database seems to be intact - computers and static groups are there, custom policies look to be copied across and in place, quarantine and threat logs seem to be there etc. The only thing I've seen so far that needed to be added, that wasn't present, was our license details under Admin -> License Management.
Once you initiated upgrade of whole appliance by pulling database from your older OVA, SERVER inside new OVA was installed, but once it started, it took some time until it was accessible from network, and that is reason why installation of AGENT failed, which resulted in OVA that was "optically" not working. It was actually almost ready for use, especially SERVER was already running. What actually helped in your case was re-configuration of new appliance, which technically executed "repair" over SERVER and finalized remaining operations. They were this time successful because SERVER was already upgraded and thus it took much less time to initialize. Updating system should not affect this issue. It is required to wait until SERVER is fully upgraded, which should not take more than an hour.
For those than experience this issue, there are few alternatives, where the easiest and recommended is to to upgrade SERVER inside old ova appliance (components upgrade task), and once this is done, and SERVER is running, migration to new OVA may be performed.
If the recommended upgrade path is still a component upgrade task from within an existing server first (which does make sense), and then migration to a new VM, if desired, perhaps the ERA v6.5 upgrade / migration instructions on the following page should be altered to reflect this?:
Datasources now store passwords and basic auth passwords in secureJsonData encrypted by default. Existing datasource with unencrypted passwords will keep working. Read the upgrade notes on how to migrate existing datasources to use encrypted storage.
Grafana v6.2 ships with a new exciting panel! This new panel, named Bar Gauge, is very similar to the currentGauge panel and shares almost all its options. The main difference is that the Bar Gauge uses both horizontal andvertical space much better and can be more efficiently stacked both vertically and horizontally. The Bar Gauge alsocomes with three unique display modes: Basic, Gradient, and Retro LED. Read thepreview article to learnmore about the design and features of this new panel.
We have been working on improving table support in our new react panels (Gauge & Bar Gauge), and this is ongoing workthat will eventually come to the new Graph, Singlestat, and Table panels we are working on. But you can see it already inthe Gauge and Bar Gauge panels. Without any config, you can visualize any number of columns or choose to visualize eachrow as its own gauge.
This has been one of the most requested features for many years and is now finally here! Lazy loading of panels meansGrafana will not issue any data queries for panels that are not visible. This will greatly reduce the loadon your data source backends when loading dashboards with many panels.
Sometimes your panels do not need a title, and having that panel header still takes up space, making singlestats andother panels look strange and have bad vertical centering. In v6.2, Grafana will allow panel content (visualizations)to use the full panel height in case there is no panel title.
Five months ago, we deprecated our old package cloud repository and replaced it with our own. We will remove the old depreciated repo on July 1. Make sure you have switched to the new repo by then. The new repository has all our old releases, so you are not required to upgrade just to switch package repository.
This is the comprehensive guide to preparing manuscripts using the AASTeX v6.2 classfile (aastex62.cls). Authors using the earlier AASTeX v6.0 classfile should use its guide as some of the functionality is different. A list of the major differences between the versions of AASTeX is available on the revision history page.
The most important aspect of the AASTeX package is that it defines the set of commands, or markup, that can be used to identify the structural elements of manuscripts. When articles are marked up using this set of standard commands, they may then be submitted electronically to the editorial office which aids both the peer review ingest and production processing while producing high quality output in a variety of styles.
This guide contains basic instructions for creating manuscripts using the AASTeX v6.2 markup package. Authors are expected to be familiar with the editorial requirements of the journals so that they can make appropriate submissions; they should also have a basic knowledge of LaTeX-for instance, knowing how to set up equations using LaTeX commands.
This section describes the commands in the AASTeX v6.2 package that an author might enter in a manuscript that is being prepared for electronic submission. The commands will be described in roughly the same order as they would appear in a manuscript. The reader will also find it helpful to examine the example files that are distributed with the package.
This specifies the document class as aastex with the default style. The manuscript copy produced by this style is a tight typeset, single column format. Other styles are available. They are discussed in greater detail in Section 3.
However, abbreviations that attempt to define new symbols by using LaTeX commands for repositioning text tend to cause problems in the publication process and should be avoided. In particular, author-defined commands that use any of the commands listed below are apt to cause problems during data conversion.
Consequently, authors are strongly discouraged from using them. In addition, AASTeX already has defined commands for all the major astronomical journals so authors should refrain from using their own as it generally leads to conflict errors during compilation.
Extra symbols are defined for AASTeX, some specifically for an astronomical context, others more broadly used in math and physics. In particular, the AMS has additional symbol fonts that are available in a standard LaTeX package (amssymb). All of these symbols are depicted in the additional symbols tables supplied with the package and on the AASTeX website.
A number of markup commands are available to timestamp important dates during the peer review process to document the publication history. These commands are not required as this information is pulled from the peer review database after acceptance and inserted by the publisher during production. Authors may find these commands useful for arXiv submissions.
The first command will print text in a light gray color on the title page running diagonally from the bottom left to the top right. The font size can also be specified by the second command, e.g. 2in, to obtain the appropriate size. Authors may have to experiment with the wording and font size to obtain a desired result. The water mark information is not used during production but authors might find it useful to identify drafts or preprints.
The way AASTeX v6.2 handles author, affiliation, and collaboration information is different from previous versions so authors should read this section carefully. There are many reasons for these changes including updates in how article titles are displayed, the addition of ORCID support, automatic affiliation indexing, improved collaboration identification, and additional article meta-data commands for preprints. The following older commands are now removed: \affil, \altaffilmark, \altaffiltext, \fullcollaborationName, and \and. LaTeX will issue an error and stop if these are encountered in an AASTeX v6.2 manuscript.
Each \author command should be have an associated \affiliation command to specify a primary affiliation. AASTeX v6.2 will automatically index all the \affiliation commands during compilation. When a duplicate \affiliation command is encountered it is given the same index number as the first \affiliation found. Physical and postal address information for the specified institution should be included with \affiliation. The address can be broken over several lines using the \\ command to indicate the line breaks. Use multiple \affiliation calls for secondary and tertiary affiliations.
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