Thursday, June 3, 2021

OPUS Update for May 2021 - New units and formats, selection of download format

It's time for another two-month update! This time we are pleased to announce a number of small features designed to increase the flexibility of how you use OPUS.

New Units and Formats

We have added new units and display formats for longitude- and latitude-like fields (including right ascension, declination, and solar hour angles). Depends on the field, you can now select:
  • Decimal degrees
  • DMS (degree-minute-second)
  • Decimal hours
  • HMS (hour-minute-second)
  • Decimal radians
DMS or HMS can be entered in various free-form formats like 12d 53' 6.23'' or 12h 30m 0s. The format is automatically detected, so even if you have selected "decimal degrees" as the unit, you can still enter the value in DMS or HMS format. If you enter a value in degrees while DMS or HMS is selected, the value is automatically converted, giving a very convenient way to convert degrees to DMS and hours to HMS (or vice versa) even if you don't plan to use OPUS to do a search! We also support a variety of Unicode characters for the degrees symbol, ', and '', which allows convenient copy-paste from web pages, including Wikipedia.

We have also added new formats to date-time fields. Dates may be entered and/or displayed as:
  • YMDhms - Year, month, day, hour, minute, second (1981-07-19T19:30:22.520)
  • YDhms - Year, day of year, hour, minute, second (1981-200T19:30:22.520)
  • Julian Date - The number of elapsed days since noon on Monday, January 1, 4713 BCE. Each period from one noon to the next counts as one day, regardless of whether that day contains leap seconds. As a result, some days are longer than others. (JD2444805.31276065)
  • Julian Ephemeris Date - Similar to SPICE Ephemeris Time but in units of days instead of seconds (JED2444805.31336462)
  • Modified Julian Date - Julian Date minus 2400000.5 (MJD44804.81276065)
  • Modified Julian Ephemeris Date - JED minus 2400000.5 (MJED44804.81336462)
  • SPICE Ephemeris Time - The time unit used by the SPICE toolkit, defined as the number of elapsed seconds since noon on January 1, 2000, and adjusted for relativistic effects that cause a clock on the Earth to vary in speed relative to one at the solar system barycenter. (-582308925.296)

Selection of Download Format

We have added a couple of options to the Download Options on the Cart tab. It is now possible to select the type of archive file (.zip, .tar, or .tgz) as well as the archive's internal file structure. The default is "flat", which is the previous behavior. With "flat" selected, all selected data products are placed in the root level of the archive file. There is a minor change though: if two different files have the same base filename, such that placing them in the root would cause a duplicate filename, they are now added to the archive using their full directory path as stored in the RMS archive. If "flat" is unselected, then all data products in the archive are stored using their full directory paths, completely mirroring the structure of the RMS archive.

Adding or Removing an Observation from the Cart on the Detail Tab

We have added the ability to add or remove an observation from the cart on the Detail tab. In addition, the header of the Detail tab is now frozen so that it is always visible.

Minor Metadata Changes

We have made a number of minor changes to the metadata and the available file products. These include fixing a bug with the wavelength of HST STIS observations and adding superseded-processing products to the available Galileo SSI download products. These changes are unlikely to be visible to most users.

As always we actively solicit your questions, feedback, and comments. Feel free to send a DM on Twitter or use the Feedback tab found on the right side of the OPUS screen, or start a chat with one of our team members. No question or comment is too small. We hope you and your family are staying safe and healthy as we all look forward to returning to a more normal life soon.

Friday, April 2, 2021

OPUS Update for March 2021 - Chat, New Data, Metadata Improvements

It's been awhile since we had an update, but we've been working hard behind the scenes on improvements. This month we're pleased to announce three basic changes: new chat functionality, new data, and improved metadata.


We really, really want to hear from you! We want to make sure you have every opportunity to ask questions and provide feedback. As such we've added a new "Chat" function. If one of the Ring-Moon Systems Node OPUS experts is available to help, you will see a Chat icon in the lower-right corner of the Search and Detail tabs. Entering your question or comment here will connect you directly to one of our team members for live help. We look forward to hearing from you.


Although there are no new missions or instruments at the moment, we did add or improve the following data sets:
  • The COISS_2xxx volumes (Cassini at Saturn) have a complete set of new calibrated data (using CISSCAL 4.0)
  • COUVIS_0xxx volumes have been updated to the latest release (version 3) and have new, improved preview images
  • COUVIS_8xxx (occultation) volumes have been updated to the latest release (version 3)
  • All occultation volumes now have preview images, and most have browse diagrams detailing occultation geometry


There have been many improvements to the RMS-generated metadata as well as a few metadata-related bugs fixed in OPUS. Metadata changes are described in new AAREADME.TXT files present in each metadata directory in the archive. Changes include:
  • For all relevant volumes, the body inventory table has been renamed from to inventory.csv to better represent its format
  • Product Creation Time has been added for most instruments
  • The Observation Type of Hubble observations has been standardized. Image is data with two spatial dimensions with each pixel containing an intensity value. Spectrum is data with zero or one spatial dimension with each pixel containing a complete spectrum. Spectral Image is data with two spatial dimensions with each pixel containing partial spectral information (usually the result of a prism or grism). Spectral Cube is data with two spatial dimensions with each pixel containing a complete spectrum. In addition, the Wavelength, Wavelength Resolution, and Spectrum Size fields have been updated to be consistent across all Hubble instruments.
  • CORSS_8xxx:
    • Several occultations that were missing from OPUS have been added
    • The format of OPUS IDs has been changed to include the "rev" number
    • The Wavelength was stored with the wrong unit and is now correct
  • COUVIS_0xxx: Data Set IDs have been updated
  • COUVIS_8xxx: Wavelength was stored with the wrong unit and is now correct
  • COVIMS_0xxx:
    • Several observations from COVIMS_0012 that were missing from OPUS have been added
    • "Packed" versions of observations have been removed when the "unpacked" versions are available
  • Many additional data product types are available for download in OPUS
    • COCIRS - Observation Metadata (ISPM)
    • CORSS - Documentation and Browse Products
    • EBROCC - Geometry Table, Preview Plot, Geometry Diagram, Source Data, and Browse Products
    • HST - HST Files Associations Index
    • VGISS - Extra Preview
  • GOSSI version 1 data products are no longer available for download through OPUS
  • HST: Data Set IDs have been updated
As always we actively solicit your questions, feedback, and comments. Feel free to send a DM on Twitter or use the Feedback tab found on the right side of the OPUS screen, or start a chat with one of our team members. No question or comment is too small. We hope you and your family are staying safe and healthy.

Tuesday, October 6, 2020

OPUS Update for September 2020 - Linked Search Fields

This month we bring you two small changes to improve the user experience: a new way to remove search fields, and linked search fields so they are easier to find.

Removing Search Fields

In the past, the only way to remove a search field on the Search tab was to click the "X" in the upper right corner. This functionality is still present, but now you can also remove a search field by clicking on the search field name on the left side of the screen as well. This mirrors the existing behavior in the Select Metadata dialog. Because it's easier to do this by accident, if you have placed any constraints on the search term you will be asked to confirm before the field is removed.

Linked Search Fields

In some cases, it may be difficult to find the metadata fields that you are interested in because they are contained in a different category. For example, when looking at occultations you are likely interested in ring radius and ring opening angle, but these fields are in the Ring Geometry Constraints category. Likewise when looking at images, you may be interested in the exposure duration, but this field is in the Image Constraints category. To make things easier for the user, we have placed "links" to some of these common fields in the places where people may expect to see them. Selecting a field in the "linked" location is exactly the same as selecting it in its native location, and both locations will be highlighted.

As always we actively solicit your questions, feedback, and comments. Feel free to send a DM on Twitter or use the Feedback tab found on the right side of the OPUS screen. No question or comment is too small. We hope you and your family are staying safe and healthy.

Tuesday, September 8, 2020

OPUS Update for August 2020 - Specifying Metadata Fields in Table View, Index Files, STIS Fields

 This month we have a new feature in Table View and a few updates to the available metadata.

Selecting Metadata Fields (Part 2)

Last month we added the ability to select metadata fields while in the Slideshow View. This month we added the ability to do the same thing while in the Table View. To add or remove a field, simply hover your mouse over the table header. A small toolbar will appear below the field you've selected. Clicking on the trashcan icon in the middle will remove the field from the selected metadata fields. Clicking on the + on the left or right of the toolbar will allow you to add a new field before or after the selected field.

Index Files as Downloadable Products

We have added our own PDS3 metadata index files ("RMS Node Augmented Index", "Supplemental Index", and "Profile Index") as downloadable products. As these are probably not needed for the average user, they are not included by default when downloading the cart contents. At the same time, we made some other product types (such as small preview images) not download by default as well. You can always explicitly select these product types if you want to include them in your download. Note there is only one set of index files for a given observation regardless the number of data versions available.

STIS Metadata Fields

We have added a new field for HST STIS: STIS Proposed Aperture Type. We have also corrected some errors in the normal Aperture Type for STIS.

As always, we thank you for using OPUS and appreciate your feedback, comments, or questions.

Friday, July 31, 2020

OPUS Update for July 2020 - Specifying Metadata Fields, Tutorial Videos, Microsoft Edge

We skipped the update for June so that we could bring you an extra-special combined update for July.

Selecting Metadata Fields

The existing Select Metadata feature (available on the Browse and Cart tabs) allows you to choose which metadata fields are displayed:

  • In the Table View
  • In the Slideshow View (when you click on a thumbnail)
  • On the Detail tab

as well as which fields are saved in downloaded CSV files. Similar functionality is now available directly in the Slideshow View. To get to the slideshow, simply click on any thumbnail in the Gallery View or any table row in the Table View. From this view, you can see a larger preview image, view the values for selected metadata fields, add observations to (or remove observations from) the cart, access a variety of features using the mini-menu in the lower right, and move to the next or previous image in your search results using the arrows in the window or the arrow keys on your keyboard.

To modify the set of metadata fields available in the Slideshow View, simply click on "Edit" at the top:

Once in "Edit" mode, you will be able to drag fields to reorder them, delete fields by clicking on the trashcan icon, or add new fields by clicking on the "+".

When finished modifying the list, click on "Done" at the top.

New Tutorial Videos

The Ring-Moon Systems Node now has a YouTube channel. We currently have two OPUS tutorials that were given at the recent OpenPlanetary virtual conference, one on how to use OPUS in the browser, and one on using the OPUS public API. The videos are also linked from the OPUS Help menu.

Support for Microsoft Edge

Microsoft has released a new version of their Edge browser, based on Chrome, which has the necessary features to support OPUS. As a result, we now consider it a supported browser.

As always, we thank you for using OPUS and appreciate your feedback, comments, or questions.

Thursday, May 21, 2020

OPUS Update for May 2020 - Occultations!

We skipped the update for April so that we could bring you an extra-special combined update for May. The short version: OPUS now supports occultation profiles!

Occultation Profiles

Four new volume sets have been added to OPUS, all containing occultation profiles of Saturn's rings:

  • CORSS_8001 (197 from Cassini RSS)
  • COUVIS_8001 (277 from Cassini UVIS)
  • COVIMS_8001 (248 from Cassini VIMS)
  • EBROCC_0001 (12 from ground-based telescopes)

To support these, there is a new Observation Type called Occultation Profile and a new Occultation Constraints section on the left side of the main Search tab:

The available search fields are:

  • Occultation Type - The type of the occultation (Radio, Solar, or Stellar)
  • Occultation Direction - The direction of the occultation through the ring plane (Ingress, Egress, or Both)
  • Body Occultation Flag - Yes or No indicating if there is a planetary or satellite body intercepted by the profile
  • Temporal Sampling Interval - The time interval between adjacent points in the profile
  • Data Quality Score - For data sets that support it, the subjective quality of the profile (Good, Fair, or Poor)
  • Detectable Optical Depth - The range of optical depths detectable in the profile
  • Wavelength Band - The wavelength of the observation (S, X, Ka, IR, Visible, or UV)
  • Signal Source Name - The source of the photons used in the profile (Cassini or the name of a star)
  • Receiver Host Name - The name of the receiver (Cassini, a DSN antenna, or one of the ground-based telescopes)

For the occultations currently available, the Intended Target Name is always Saturn Rings. For the ground-based occultations, the Mission is Ground-based and the Instrument Name is the name of the ground-based telescope.

Other search fields relevant to occultations can be found in other categories:

  • Wavelength Constraints includes information on the actual wavelengths used to create the profile
  • Ring Geometry Constraints includes information about incidence, emission, and ring opening angle, ring radius range, ring longitude range, and ring resolution
  • Cassini Mission Constraints, Cassini UVIS Constraints, and Cassini VIMS Constraints, as appropriate, include information about the raw observations that were used to make the profile

Most occultation profiles are available in multiple resolutions. All of these versions are combined together into a single OPUS observation. Which resolution(s) you want to actually download can be selected on the Cart tab:

Note that there are no thumbnail preview images for occultation profiles at this time (but we hope to generate them soon), so we suggest you browse your search results in the Table View.

Other Miscellaneous Changes

We implemented a few other minor interface changes and bug fixes in the metadata in this release that will probably be invisible to most users, but are listed here for completeness:

  • Selections that are not relevant are now called "N/A" instead of "NULL".
  • We changed all Ring Geometry Constraints "body center" metadata fields into "range" fields (with a minimum and maximum stored in the database) to support the ranges available for occultation profiles. These fields now support the "any/all/only" query types, although for non-occultation observations the minimum and maximum will always be the same for a given observation. In the future, all ring geometry will be regenerated so that these fields have appropriate ranges of values.
  • The Surface Geometry Constraints / Multiple Target List metadata field is now in title case instead of all upper case.
  • We fixed a problem with Cassini UVIS HSP observations where they had the wrong duration and stop time.
  • We changed Cassini VIMS IR and Visual exposure durations to be in units of seconds instead of milliseconds to be consistent with all other duration fields

As always, we hope you and yours are safe during these trying times, and we look forward to hearing your comments, questions, and suggestions.

Tuesday, March 31, 2020

OPUS Update for March 2020 - Sort on Multiple Fields, Improved Mobile Support

As we continue in these challenging times, we hope you will enjoy some of the new features we've provided for you this month:

  • The ability to sort on more than one metadata field at a time
  • Improved support for small mobile devices and tablets
  • A minor change to the Multiple Target List field to make your life easier

Multiple-Field Sort

There are many cases where sorting on a single metadata field is not enough to give you the ordering you might want. For example, if you sort on Planet, you have no control over what order the observations for a particular planet are presented in. OPUS has always added OPUS ID as a second sort field to guarantee determinism in the results, but what if you wanted to search first on Planet, then for a given planet on Instrument Name, then for a given Planet+Instrument Name on Intended Target Name, and then for a given Planet+Instrument Name+Intended Target Name on Observation Start Time? The OPUS API has supported this ability for awhile, but now the UI does too!

The current sort fields are presented near the top of the Browse and Cart tabs. The same sort order is used for both tabs, and for both the Gallery and Table views.

Each sort field is shown in order; OPUS ID is always required and must be the last field, so it is shown to the right of a vertical divider. The sort direction for each field can be flipped between ascending and descending by clicking on the field name and the arrows show the direction chosen (down is ascending and up is descending, representing how the observations will be displayed). All sort fields except the final OPUS ID can removed by clicking on the X.

To add a new field (maximum 9), click on the +. You will be presented with a drop-down list of all of the unused fields you have currently selected using Select Metadata. The new field you select will be added at the end of the list (but before OPUS ID). If you want to sort on a field that isn't shown, you need to first add it to the available list using Select Metadata. Once you've added a field to the sort order, you can remove it from the displayed fields using Select Metadata if you'd rather not see the value in the slideshow or table. You can also reorder the fields with drag-and-drop. Using these techniques we can produce the sort order discussed above:

In the Table view, each table header field that is in the sort order has a small number inside a circle. This number represents the position of that field in the sort order list. If a field is in the sort order, you can click on the table header for that field to flip its sort direction. If a field is not in the sort order, you can click on the table header to sort on that field. If there are only two or fewer fields (including OPUS ID) currently being sorted on, clicking on a table header field will replace the current sort with that field. This gives the same behavior that OPUS had previously. However, if there are more than two fields, you will be asked if you want to append the field you clicked on to the end of the sort order, or if you want to replace the entire sort order with that single field. Using Ctrl+click on a table header field is a short cut to append the field to the end of the sort order.

If you would like to reset the sort order to the default (Observation Start Time, OPUS ID), simply click on Sort by or its icon.

Improved Mobile Support

OPUS is now much more responsive and is usable in smaller browsers, all the way down to the size of an iPhone 5. As browser size decreases, some features (such as download links and feedback) are inaccessible because they make the screen too crowded and are unlikely to be used on a small mobile device anyway. Note that Safari (the default browser) on iOS has "features" (such as hiding and showing the URL navigation bar, and allowing pull-to-refresh even when there's nothing to refresh) that make using OPUS more difficult, and there is no way around these "features". If you want to have a better experience using OPUS on an iOS device, we suggest using Chrome instead.

Here is what OPUS looks like now on an iPhone 7:

As always, we welcome your feedback. Stay safe everyone.

Friday, March 6, 2020

OPUS Update for February 2020 - Search by Regular Expression, New Multiple Target List Field

Happy February everyone! We at the PDS Ring-Moon Systems Node hope that you and your loved ones are safe and that your lives have not been unduly disrupted by recent events.

This month we have two big new features for you, as well as a couple of small ones:

  • The ability to search on string fields using regular expressions
  • A new Multiple Target List field for searching on targets in the field of view
  • Tooltips are now available on touchscreen-only devices
  • You can copy-and-paste the green hinting numbers

Regular Expressions

There are a variety of ways to search for strings:

  • contains - The metadata field contains the search string somewhere within it
  • begins - The metadata field starts with the search string
  • ends - The metadata field ends with the search string
  • matches - The metadata field matches the search string exactly
  • excludes - The metadata field does not contain the search string

To these we have added a new one:

  • regex - The metadata field matches the given regular expression

For example, let's say you would like to search for all COISS volumes 2013 thru 2018. Before you would've needed to use the recently-added multiple search functionality:

but now you can simplify it into a single search:

We implemented regular expressions using the full-featured ICU library, which supports just about every regular expression feature you could want. For example, you could use "(?!COISS_2015)COISS_201[3-8]" to search for every volume COISS_2013 thru COISS_2018 except for COISS_2015. Please note that, by default, regular expressions are not anchored and the search string can appear anywhere in the metadata field. If you want to make sure that the regular expression is the only thing in the field, you can start it with "^" (anchor left) and end it with "$" (anchor right): "^COISS_201[3-8]$". Also, string fields now support input validation just like numeric fields do. If you select the "regex" query type, then your regular expression will be validated as you type it. An illegal regular expression (for example mismatched parentheses) will have a yellow border until you fix it; a legal regular expression will have a green border.

The Multiple Target List Field

There is a new field under Surface Geometry Constraints called Multiple Target List. For every observation for which surface geometry is available (currently Cassini ISS, UVIS, and VIMS, New Horizons LORRI, and Voyager ISS) this field contains a comma-separated list of every body in the field of view in alphabetical order. For example, if an image contains Rhea, Tethys, and Saturn, the field will be "RHEA,SATURN,TETHYS". There are two main uses for this. The first is for easily displaying what body(ies) you are looking at in an observation. For this you can add Multiple Target List to your Selected Metadata. The second is for searching for observations that contain specific bodies. For example, there are Cassini ISS images containing only Rhea and Tethys. To search for them, you could use "RHEA,TETHYS" with the "matches" query type.

You can also combine the Multiple Target List field with regular expression searching to get more sophisticated searches. If you would like every image that contains exactly two bodies, you can use "^\w+,\w+$". If you want one of those bodies to be Rhea, you could do two searches, one on "^RHEA,\w+$" and the other on "^\w+,RHEA$". Here is an example of a search for all Cassini ISS images that contain Rhea plus one other body, where that other body is not Saturn, and where Rhea is reasonably-sized in the image (resolution 3-10 km/pixel):

As always, we welcome your feedback, comments, and questions and look forward to hearing from you.

Tuesday, January 28, 2020

OPUS Update for January 2020 - Add All to Cart, New API Guide, and Much More

This month we are pleased to introduce a host of improvements, including:

  • The ability to add all current results to the cart
  • Thumbnails in the table view
  • Improved handling of surface geometry target constraints
  • A new API Guide and minor changes to the API itself
  • Support for directly creating PDF files from the Help menu
  • New search fields for HST STIS and Cassini
  • A change to HST OPUS IDs

There's a lot to cover, so let's get started!

Add All Results to Cart

In addition to the current ways of adding a single observation to the cart (Ctrl+Click, the shopping cart icon in the gallery view / checkbox in the table view, or the Add to Cart menu option) or multiple observations to the cart (Shift+Click to select the start and end of the range or the Start Add Range menu option), it is now possible to add all of the observations in the current search results to the cart. This is useful if you have narrowed your search to just the observations you care about downloading. Note that there is a limit of 10,000 observations in the cart, so you must add search constraints to get your result set down below this number before attempting to add them.

There are two ways to add all of the current observations to the cart. The first is the Add all results to cart menu available on any thumbnail or table row; it doesn't matter which observation you use as they all do the same thing. The second is the shopping cart icon available at the left edge of the header of the table view. Both will ask for confirmation before performing the operation.

Thumbnails in the Table View

Rows in the table view now contain a small thumbnail to the right of the cart checkbox and menu. This thumbnail can be enlarged by simply hovering your mouse over it.

Improved Handling of Surface Geometry Constraints

Surface Geometry fields are available by selecting a Surface Geometry Target Name under the Surface Geometry Constraints category. Only one surface geometry target can be selected at a time. Now, when you change the surface geometry target, all of the search fields related to the previous target that you created will automatically switch to the new target while keeping their old search values. This is useful if, for example, you are looking for observations of a set of moons at a particular range of phase angles. Just choose your first target, set the phase angle range, and add all of those observations to your cart. Then change the target and the same phase angle range will automatically be used for the new target. Then you can add all of those observations to the cart as well.

In addition, when you change targets your list of selected metadata fields will automatically be updated. If you have any fields related to the current target, then when you change targets a new set of fields for the same metadata fill be added for the new target.

For example, let's start with high phase angle and high resolution images of Enceladus and select a few metadata fields:

Now let's change the target to Titan:

Note that when performing the search, all surface geometry targets other than the one selected have "--" as their result count. Normally a number is provided that tells you how many results will be available if you select the given option. However, in this case selecting an option actually changes other search fields, so such a number is much harder to compute and is confusing to interpret so it is not provided.

New API Guide and API Changes

OPUS provides a comprehensive API for third-party applications to search its database and retrieve information. The associated API Guide has been completely rewritten. It is now much more complete and easier to read. It is available under the Help menu or directly from

The API itself has also undergone minor changes to make it more consistent. Most of these changes will not affect current users, and in many cases backwards compatibility is provided. Please refer to the API Guide for the most authoritative description of the API calls and the format of their return values.

Creation of PDF Files

Most documents available under the Help menu now allow you to create and download a PDF version. This PDF version is created live and is always up-to-date with the current version of OPUS.

New Search Fields for HST STIS and Cassini

There are two new search fields:
  • STIS Optical Element under Hubble Mission Constraints gives the optical element (grating, mirror, or prism) used for an HST STIS observation. It is NULL for all other instruments.
  • Cassini Original Target Name under Cassini Mission Constraints gives the original TARGET_NAME field supplied by the instrument teams. The meaning of this field varies by instrument and observation and should only be used by researchers familiar with these details. Normally, Intended Target Name gives a better representation of the actual primary target of the observation. OPUS creates Intended Target Name from a variety of sources to give the most useful results for most researchers.

Change to HST OPUS IDs

All HST OPUS IDs now include the full 9-character filename. This was done to make interaction with the MAST archive more seamless.

As always, we actively solicit all feedback, comments, and suggestions.

Thursday, December 19, 2019

OPUS Update for December 2019 - User-Selectable Units and More

This month we are pleased to introduce a major new feature: user-selectable units during search. We have also made some minor improvements to the Select Metadata dialog, made minor adjustments to the OPUS IDs for Hubble observations, and made minor changes to the product types available for download.

User-Selectable Units

Many search fields now allow the user to select which units to use for the input values. For example, Observed Ring Radius is usually in units of "km". However, it is now possible to select other distance units such as "m", "Rj" (Jupiter radii), or "Rs" (Saturn radii). Time fields (like Observation Duration) are normally in units of "secs". However, it is now possible to select other time units such as "msecs", "minutes", "hours", or "days". To select a unit, simply use the dropdown box at the top of the search box:

Preprogrammed ranges (Wavelength and Observed Ring Radius) will be presented in the selected units.

If there are already values entered into any of the input fields, they will automatically be converted when a new unit is selected. Only one unit can be selected for all of the input fields for a particular metadata field.

Note that when viewing metadata fields, such as on the Detail tab or in the slideshow or table views, the data will always be presented in its native units, not the units selected for search.

Select Metadata Enhancements

In the Select Metadata dialog, any metadata fields that have been selected on the Search tab will be presented first. This is an attempt to make your experience more efficient by assuming that if you're searching on a particular field, you probably also want to see that field displayed when you view the metadata. The fields presented under Current Search Fields will also be shown under their respective categories, and can be selected or deselected in either location.

In addition, it is now possible to download a CSV file directly from the Select Metadata dialog using the currently chosen fields, even if those fields haven't been "saved" as a permanent selection. This makes it easier to download a CSV file containing particular fields without pressing additional buttons, and also allows you to download a CSV file containing fields that you don't normally want to see in the OPUS UI (by downloading but not saving the field changes). If you are viewing the Browse tab, the CSV file will contain all of the current search results. If you are viewing the Cart tab, the CSV file will contain all items in the main cart (not in the recycle bin).

Hubble OPUS IDs

A small number of Hubble observations have multiple versions that were downlinked at different times. In these cases we make the filename portion of the OPUS ID 9 characters instead of 8 to allow the observations to be distinguished. This has slightly increased the number of NICMOS observations available.

Download Product Types

Some New Horizons observations have multiple versions that were downlinked in different formats but are otherwise identical. We provide the highest-quality versions as Raw Image or Calibrated Image and now provide all additional versions together as Raw Image Alternate Downlink or Calibrated Image Alternate Downlink. Also, the list of product types has been reversed, placing the most important types (e.g. actual mission data) first and secondary data (inventory files, preview images) last. 

Happy Holidays from the OPUS team (Rob, Dave, and Debby) and we look forward to serving you in the New Year. As always, we actively solicit all feedback, comments, and suggestions.