Do you use the IAS Viewer to view our JPEG2000 (JP2) image files at full-resolution (which we highly recommend!)? If you use a Mac running OSX, you might be having trouble. Don’t worry, there’s a solution!

It appears that a recent Java patch causes problems launching the IAS Viewer client and other Java-based software launched via Java Web Start. The update changed the location of the Java Web Start application so that the system opens the downloaded JNLP file as a text file, most likely with something called Dashcode. One of our system administrators found a solution on an Apple support discussion archive. You should only have to do this once to fix the problem:

(more…)

Spacecraft missions are complicated endeavors that result in a wealth of scientific and engineering data. Long after the mission has ended, these data can be extremely useful for later study and discovery. With so many missions over so many years, how can later generations find and make use of these data?

The solution for many NASA missions has been the development of the centralized Planetary Data System (PDS). The PDS is several things: a collection of websites, a search capability, an archive, a database, a learning tool, etc. The PDS Imaging Node is located at http://pds-imaging.jpl.nasa.gov/ and acts as “the curator of NASA’s primary digital image collections from past, present and future planetary missions.” These missions include Voyager, Galileo, Cassini, and many more. Now the Mars Reconnaissance Orbiter (MRO) has been added to the list, with the HiRISE team releasing our first several months of image data.

• MRO PDS page: http://pds-imaging.jpl.nasa.gov/Missions/MRO_mission.html
• MRO Product Search page: http://pds-imaging.jpl.nasa.gov/search/index.jsp
• HiRISE Volume: http://hirise-pds.lpl.arizona.edu/PDS/

What we have released is an archive of the HiRISE Experiment Data Records (EDRs) and Reduced Data Records (RDRs). EDRs are in the *.IMG file format and represent individual CCD channels (remember, there are 14 CCDs in the HiRISE camera and two channels per CCD, for a total of 28 channels). These EDRs are cleaned up, calibrated, stitched together, and mapped to Mars’ geometry, resulting in the RDR products. RDRs are in the *.JP2 and *.LBL formats. JPEG2000 is the technology that enables us to offer our gigantic images to the scientific community and the public in a timely and efficient manner. An observation’s image data are in the *.JP2 file and its meta data are in the detached *.LBL files. To view these products, JPEG2000 compatible software is required (see our site for a list of offerings).

While we have been trying to release up to five captioned images a week for the past few months, the PDS release represents several hundred images, most of them without captions. You can find them using the PDS search capabilities, and you can also find them on the new HiRISE site, unveiled today to coincide with this first PDS release. The redesigned site focuses on the images while providing, hopefully, a more user-friendly interface:

• HiRISE Site: http://hirise.lpl.arizona.edu/
• “About Our Redesign”: http://hirise.lpl.arizona.edu/profil.php
• Images released to the PDS: http://hirise.lpl.arizona.edu/pds_release.php

As word gets out about the new site and the PDS release, you may experience some site slowness. Please be patient, and thank you for your interest!

Tuvas posted this great top-ten list over on Unmanned Spaceflight.

I changed it around a bit, hope you don’t mind, T!

1. You consider any image with less than a billion pixels a mere pittance… a negligible amount of data.
2. You realize that any part of Mars can be interesting, if viewed at sufficiently high resolution.
3. You start to see in black and white away from the “Center strip” of your eyes.
4. You have decided to buy a 500 Gigabyte drive just to store a few dozen of your favorite HiRISE Images.
5. You’re considering getting a new 40″ LCD mainly to look at HiRISE Images.
6. You know what JPEG 2000 is.
7. You start making up new Hi Names (HiStuff, HiSpace, etc, etc).
8. You continually refresh the web page starting Wednesday morning, waiting for the next release.
9. When using Google Earth, you wish you could zoom in further, just like HiRISE can.
10. You’re reading this!

To conclude our exploration of the pipelines that take raw channel files and create a beautiful, unmapped mosaic, let me introduce the Stitch pipelines: HiStitch and HiccdStitch.

The HiStitch pipeline combines the matching HiCal products for the same CCD into one more-or-less lined up CCD cube file. HiccdStitch combines these HiStitch cubes into RED, IR, and BG mosaics.

Both pipelines take some time, as overlapping pixels are accounted for and brought together. After these mosaics are created, additional steps create smaller jpeg files for easier viewing, and full-sized jpeg2000 files. We use these jpeg2000 files for validating our images.

There are later pipelines, but we first validate the HiccdStitch products: Did the previous pipelines work correctly? Did the uplink team command the camera correctly? Is there haze or clouds obscuring our view of the surface?

If everything looks good, and we have received the correct reconstructed SPICE ephemeris data, then the geometry pipelines are invoked. These pipelines project the images mathematically to a model of Mars and add geometry data to the images so that each pixel becomes a point on Mars with latitude and longitude coordinates.

Well, it’s been a while since we’ve been posting a lot, so I thought I’d just give you guys some kind of an idea as to what we’re doing these days.

The uplink team is constantly looking where to point the camera next. There is a program which is in beta testing now called HiWeb which allows scientists and other people to input suggestions. The Uplink team reviews the suggestions in the database, assigns a priority to each of these suggestions, and then finds when we can point the camera at the part. They also make sure a certain percentage of the upcoming pictures are assigned to look for a Phoenix landing spot, as this is a high priority item at the moment. They are still learning exactly how to best command the camera, and are constantly sharpening their skills.

The downlink team is making sure operations run smoothly at HiROC. They are verifying that the processing has taken place, make sure that the images have been calibrated correctly, that there are no image processing artifacts on the images we are about to release. If there is any artifacts created from processing the image, the source of the problem is identified and fixed, and then the image is reprocessed. While previously we have sent images to the public that had some small processing artifacts during the post-MOI and Transition imaging, we currently are waiting until the images have been completely validated. The downlink team is also taking a quick look at each image that comes down, and making sure there isn’t something unexpected, for example, haze at Mars, lots of saturated pixels, etc. If any such problems are found, they notify the uplink team, to ensure that we don’t have continuing problems. These problems are very rare, but on occasion happen, due to the changing nature of Mars. (more…)

Twelve delightful images for your viewing pleasure are now available. I’m also starting a page answering JPEG-2000 questions, keep sending them in!

Here we are over two weeks into PSP, and we haven’t even finished releasing our TRA images!

Actually, today we got 31 TRA images out the door, just about completing that set. In addition, the previous 32 grayscale images have been reprocessed with our improved geometry—no more jagged edges on the reprojected “Red Mosaics”.

Furthermore, the full-res images are now available as lossless JPEG-2000 (JP2) files. At HiROC we are using the ExpressView application from a company called LizardTech… a subsidiary of some Japanese company (that has no affiliation to us FWIW).

ExpressView is available for Mac and Windows. Their download page describes it only as a browser plug-in, but the installer contains an application as well.

ExpressView provides progressive rendering (though you still have to have the entire file first—we are considering moving to a streaming model using the JPIP protocol but there are even fewer clients available). It should also reduce the amount of memory (RAM) needed to view our largest images.

There are a few options available to Linux users, but nothing we have tried is as fast or as feature-rich. In any case, let us know what works or doesn’t work for you.

All of these images are available at the usual location.

A system for streamlining the process of editing captions, highlighting cut-out areas and pushing out web pages is in the works. We will get caught up.

In the meantime, look for the first set of PSP releases by this time next week.

P.S. Happy Thanksgiving.

The first HiRISE image data of the Primary Science Phase (PSP) arrived in Tucson last night sometime around 9 PM. Although we thought the first data might not arrive until early this morning, I was a little antsy and took a look from home around 9:40 PM to see a complete first observation ready for validation.

We are waiting for reconstructed SPICE ephemeris data, which comes out every Wednesday – starting next week – before sending these data through our geometry pipelines, and ultimately releasing them to the scientific community and public. Last time, we forced images through our geometry pipelines using predicted SPICE kernels; we do not want to double our workload by continuing that practice. The SPICE kernels released next Wednesday will cover some of the images captured this week.

Once the images have been visually and statistically validated and the matching SPICE kernels have arrived, one of the downlink folks will send the images through the geometry pipelines. We also need to get a select group of captions written and automatic caption information generated for the rest.

We are producing JPEG2000 products now in addition to smaller jpeg browse images, to be ready for our viewing client when it is ready for public release. However, there are many different JPEG2000 viewers and plugins already out there to start practicing with. One example is ExpressView from LizardTech.

Once we are on a roll, the data release will be steady and no one will be able to keep up with the wealth of Mars data coming in. Until the first public release of PSP images, we will try to provide here on HiBlog more details about the many tasks that must still be completed.

While most of our uplink and downlink procedures have been developed and tested fairly heavily over the last year and a half, we still have parts of our ground data system that are in heavy development. The distribution of our imaging products to the Planetary Data System’s Image Atlas, our scientific colleagues, and you, the public at large is still very much a work in progress. Through the month of October I have been developing the next part of our PDS data node culminating in a test where I practiced the release of 2 days worth of imaging products from our Post Mars Orbital Insertion imaging campaign back in March. For the purposes of this test I released 196 raw products and our first sample JPEG2000 product.

(more…)

Some of you out there may be asking: what happens to a HiRISE image between the time that it is taken and the time that it is released to the public? Well, I’d like to give a summary here.

(more…)