We have now released all HiRISE images taken prior to August’s spacecraft safe mode event! Here are some statistics about our October 2009 release, which includes the images the HiRISE camera took of the Martian surface between Mars Reconnaissance Orbiter (MRO) orbits 14,200 to 14,499 (August 6, 2009 – August 26, 2009):

• 446 RDRs, 0.18 TB
• 6238 EDRs, 0.18 TB
• 5126 RDR Extras, 0.28 TB
• 12,464 EDR Extras 2.5 GB
• 16 Anaglyphs 0.001 TB

Totals for this release: 24,274 images, 0.62 TB

This brings our total released product numbers and data volume to:

• 23,122 RDRs, 12.2 TB
• 323,358 EDRs, 10.6 TB
• 196,058 RDR Extras, 15.6 TB
• 625,233, EDR Extras, 0.1 TB
• 1,192 Anaglyphs 0.5 TB

Total: 1,167,771 images, 37.7 TB

Just because we are not currently taking images does not mean we are slacking off. The Downlink team is busy reprocessing and validating all ESP observations. After reprocessing, these observations will all benefit from the same improvements we have made to our processing pipelines over the past several months. I also recently started reprocessing PSP observations, which is a much larger data set that will sync improvement to our processing pipelines made over the past few years! We are keeping busy and we are even getting help from the Uplink team while they wait for the go ahead to start taking new images of the Martian surface. Of course we all want that to happen as quickly as possible!

The first few cycles of the extended science phase (ESP) have been very similar to the previous primary science phase (PSP). The main difference has been that the Observation IDs start with ESP instead of PSP! (like ESP_011268_2485) We’re also adding some warm-up observations on the night side of the planet now, which is adding some extra work in the planning. Luckily (?), Mars is at its farthest distance from the Earth right now, so the data rate is very low. This means fewer images to plan, so we have some extra time to do special things like this.

The next cycle, however, will mark some changes in the way we do the planning process. This is cycle 58 (can you believe it’s been that many cycles since we started??). For most of that time, we’ve been doing things in much the same way. We’ve gotten so good at it that everyone decided they wanted to change everything & mess it all up. haha, just kidding. We’re actually trying to simplify things. Even though we’ve gotten pretty good at this, it’s still an incredibly complex process. We would like to continue doing it for a long time and still remain sane. Also, we expect that our funding will be cut in the future, and we want to make sure we can still do everything even if we have fewer people. Plus, things just wouldn’t feel right if we weren’t constantly changing something!

If you’re interested in the nitty-gritty details, here are some of the things we’re changing: (more…)

We’re in the midst of the last cycle in MRO’s Primary Science Phase (PSP). Conjunction is coming up, when Mars is behind the Sun, so we won’t be able to communicate with the spacecraft for a few weeks. We’ll get a welcome break during that time – Uplink will have two whole planning cycles off, and Downlink will get a chance to catch up with their processing.

I can’t believe it’s been two years since the last conjunction and the start of PSP! A lot has changed since we started out with those first images. (more…)

Here are 40 RGB color images from the 1500 – 1600 orbit range of MRO.

View Images

There are, as always, many magnificent images here. Some of the noteworthy observations are:

PSP_001521_2025 and PSP_001501_2280: On the HiRISE web site you can see diagrams made by Tim Parker show the locations of various parts (lander, backshell, heatshield or parachute) for Viking Lander 1 and Viking Lander 2. It’s possible they aren’t in the color strip (I haven’t found them)!

PSP_001508_1245 and PSP_001510_2195: These two exhibit a “glow” pattern of saturated pixels due to high TDI (Time Delay Integration) settings on the blue-green CCDs. (All of the exposure settings are chosen for each observation based on a photometric model of the scene).

PSP_001538_2035: This is a rim-to-rim section across a crater called Tooting that is about 30 kilometers in diameter. It’s also interesting to note how the altitude of the rims, when combined with the large off-nadir roll angle (23 degrees), leads to an oddly bowed geometric projection. But it is correct; as the terrain rose, fell, and rose again from HiRISE’s angled point of view, the center of the ground track deviated slightly east or west from a true great-circle line.

PSP_001558_1325 and PSP_001593_2635: These dune fields are striking, forming incredible patterns.

PSP_001582_2245: Looking like a super-sized area of dried mud, the polygonal cracks in this image are amazing.

Updated (2008-Apr-10)

If HiRISE is like, well, a high rise, then each orbit range is a floor. The thirteenth floor consists of observations in the range 1300 to 1399. These were our first images of Primary Science Phase.

Click the link below to view a gallery of 50 HiRISE images in the 1300 range, drawn from our online PDS data node. The RGB browse is shown in the window, linked to the full JPEG 2000 using the IAS viewer. The RGB browse scale image is usually scaled down by a factor of 8–in both horizontal and vertical directions–from the JP2 product. So the browse image shows you around 1/64th of the color data: there are vast and beautiful scenes that can only be seen in full by zooming in with IAS. Nevertheless, if you have some time, this is a good way to explore a set of images and get an overall idea of what there is to see.

View Images

Most images are several times taller than your computer screen, so make sure to scroll through each one. Let us know which images are you favorite via the comments form below.

Updated (2008-Apr-10)

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…)

Tomorrow marks the beginning of the third two-week cycle in the primary mission. However, it’s only my first cycle! One Targeting Specialist is assigned to each cycle, and I’m on for cycle 3. Because we spend almost four weeks planning before the cycle even starts, there are three Targeting Specialists overlapping at any one time, in various stages of the planning process. Plus there’s a backup — HiBUTS, which stands for HiRISE BackUp Targeting Specialist. (I can’t take credit for that — that’s one of HiKu’s!)

Since before PSP started, we’ve all been working long hours. We haven’t had much time to blog, but right now I’m just waiting nervously for my commands to be radiated, so I thought I’d share this recipe. For all you faithful blog readers out there (all 2 of you? ), here’s my secret to surviving long workdays and cold nights:

(more…)

PSP Image 1440-1255 shows a network of gully-like channels on the sides of dunes inside Russell Crater. On the sunward side, the channels are long and continuous, terminating at the base of the dunes. On the more shadowed side, strange stipples interrupt the otherwise silky smooth dune faces, as if the channel forming process never quite gets going.

Aside from the scientific significance of this image—which hopefully can tell us how these features formed and how recently—it is one sexybeautiful image, and my personal favorite so far!

This image and twelve others were released today; the first set of Primary Science Phase images from HiRISE.

At about 11:34 UTC, DSN received a transmission from MRO that HiRISE was successfully turned on, after the end of the solar conjunction. This marks the official start of the Primary Science Phase (PSP) of HiRISE, and MRO in general. During this time we expect to image 1-2% of Mars in high resolution. Starting late Tuesday evening/early Wednesday morning, we will begin to receive pictures from Mars, without much of a pause for some time to come.

I would just like to offer my thanks to all of those who helped to make HiRISE at Ball Aerospace, the flight engineers at JPL, operations team, programmers, targeting specialists, scientists, and everyone else involved in the project. The long period of preparation is over, and now we begin with the real thing. Have a fun 2-year PSP all!

A few of us were at HiROC Saturday, getting our parts of the operations process in order for the upcoming start of primary science (PSP).

That’s GuyMac on the left, HiCommander (me!) in the middle, and HiKu on the right.

(more…)