The “Group” indicator in FSL

In FSL, when we create a design using the graphical interface in FEAT, or with the command Glm, we are given the opportunity to define, at the higher-level, the “Group” to which each observation belongs. When the design is saved, the information from this setting is stored in a text file named something as “design.grp”. This file, and thus the group setting, takes different roles depending whether the analysis is used in FEAT itself, in PALM, or in randomise.

What can be confusing sometimes is that, in all three cases, the “Group” indicator does not refer to experimental or observational group of any sort. Instead, it refers to variance groups (VG) in FEAT, to exchangeability blocks (EB) in randomise, and to either VG or EB in PALM, depending on whether the file is supplied with the options -vg or -eb.

In FEAT, unless there is reason to suspect (or assume) that the variances for different observations are not equal, all subjects should belong to group “1”. If variance groups are defined, then these are taken into account when the variances are estimated. This is only possible if the design matrix is “separable”, that is, it must be such that, if the observations are sorted by group, the design can be constructed by direct sum (i.e., block-diagonal concatenation) of the design matrices for each group separately. A design is not separable if any explanatory variable (EV) present in the model crosses the group borders (see figure below). Contrasts, however, can encompass variables that are defined across multiple VGs.

The variance groups not necessarily must match the experimental observational groups that may exist in the design (for example, in a comparison of patients and controls, the variance groups may be formed based on the sex of the subjects, or another discrete variable, as opposed to the diagnostic category). Moreover, the variance groups can be defined even if all variables in the model are continuous.

In randomise, the same “Group” setting can be supplied with the option -e design.grp, thus defining exchangeability blocks. Observations within a block can only be permuted with other observations within that same block. If the option --permuteBlocks is also supplied, then the EBs must be of the same size, and the blocks as a whole are instead then permuted. Randomise does not use the concept of variance group, and all observations are always members of the same single VG.

In PALM, using -eb design.grp has the same effect that -e design.grp has in randomise. Further using the option -whole is equivalent to using --permuteBlocks in randomise. It is also possible to use together -whole and -within, meaning that the blocks as a whole are shuffled, and further, observations within block are be shuffled. In PALM the file supplied with the option -eb can have multiple columns, indicating multi-level exchangeability blocks, which are useful in designs with more complex dependence between observations. Using -vg design.grp causes PALM to use the v– or G-statistic, which are replacements for the t– and F-statistics respectively for the cases of heterogeneous variances. Although VG and EB are not the same thing, and may not always match each other, the VGs can be defined from the EBs, as exchangeability implies that some observations must have same variance, otherwise permutations are not possible. The option -vg auto defines the variance groups from the EBs, even for quite complicated cases.

In both FEAT and PALM, defining VGs will only make a difference if such variance groups are not balanced, i.e., do not have the same number of observations, since heteroscedasticity (different variances) only matter in these cases. If the groups have the same size, all subjects can be allocated to a single VG (e.g., all “1”).

Better statistics, faster

Faster permutation inference

Permutation tests are more robust and help to make scientific results more reproducible by depending on fewer assumptions. However, they are computationally intensive as recomputing a model thousands of times can be slow. The purpose of this post is to briefly list some options available for speeding up permutation.

Firstly, no speed-ups may be needed: for small sample sizes, or low resolutions, or small regions of interest, a permutation test can run in a matter of minutes. For larger data, however, accelerations may be of use. One option is acceleration through parallel processing or GPUs (for example applications of the latter, see Eklund et al., 2012, Eklund et al., 2013 and Hernández et al., 2013; references below), though this does require specialised implementation. Another option is to reduce the computational burden by exploiting the properties of the statistics and their distributions. A menu of options includes:

  • Do few permutations (shorthand name: fewperms). The results remain valid on average, although the p-values will have higher variability.
  • Keep permuting until a fixed number of permutations with statistic larger than the unpermuted is found (a.k.a., negative binomial; shorthand name: negbin).
  • Do a few permutations, then approximate the tail of the permutation distribution by fitting a generalised Pareto distribution to its tail (shorthand name: tail).
  • Approximate the permutation distribution with a gamma distribution, using simple properties of the test statistic itself, amazingly not requiring any permutations at all (shorthand name: noperm).
  • Do a few permutations, then approximate the full permutation distribution by fitting a gamma distribution (shorthand name: gamma).
  • Run permutations on only a few voxels, then fill the missing ones using low-rank matrix completion theory (shorthand name: lowrank).

These strategies allow accelerations >100x, yielding nearly identical results as in the non-accelerated case. Some, such as tail approximation, are generic enough to be used nearly all the most common scenarios, including univariate and multivariate tests, spatial statistics, and for correction for multiple testing.

In addition to accelerating permutation tests, some of these strategies, such as tail and noperm, allow continuous p-values to be found, and refine the p-values far into the tail of the distribution, thus avoiding the usual discreteness of p-values, which can be a problem in some applications if too few permutations are done.

These methods are available in the tool PALM — Permutation Analysis of Linear Models — and the complete description, evaluation, and application to the re-analysis of a voxel-based morphometry study (Douaud et al., 2007) have been just published in Winkler et al., 2016 (for the Supplementary Material, click here). The paper includes a flow chart prescribing these various approaches for each case, reproduced below.

Faster permutation inference

The hope is that these accelerations will facilitate the use of permutation tests and, if used in combination with hardware and/or software improvements, can further expedite computation leaving little reason not to use these tests.

References

Contributed to this post: Tom Nichols, Ged Ridgway.

FSL on the Raspberry Pi


How about processing brain imaging data on a Raspberry Pi? The different versions of this little device have performed exceptionally well for education, entertainment, and for a variety of do-it-yourself projects, with many examples listed in websites such as Instructables and Adafruit. Most of these applications are not computationally as intensive. Yet, the small size, low power consumption, improved hardware in recent models, and low price, may make this feasible.

The Pi 2

Released earlier this year, the Raspberry Pi 2 (Model B) features a quad-core 900 MHz ARM processor, 1 GB of RAM, GPU, 4 USB ports, 10/100 Mbps Ethernet, HDMI and audio outputs, camera and display ports, as well as a low level general purpose interface (GPIO), all in a portable board of 85.6 mm × 56.5 mm (the same size as a credit card). It is powered by a 5 V, 800 mA DC (4 W) source, and sold for £30 or less.

Differently than earlier models, which had a CPU based on the ARMv6, the Pi 2 uses an ARM Cortex-A7 processor, which on its turn based on the ARMv7 architecture. Although there are Linux distributions that can run on the earlier models (such as ports of DebianopenSUSE, and Fedora), this change widens potential applications, not only because there are more ports available for ARMv7 (e.g., openSUSEDebianCentOS, among others), but also, the higher performance suggests that somewhat heavier data processing can be considered.

It is also possible to assemble multiple Pis in a cluster, using distributed computing engines such as SLURM, TORQUE or SGE. The Pi has the core requisites: it runs on Linux and comes with a decent 10/100 Mbps Ethernet port, such that creating a system is a matter of assembling the pieces and configuring.

Neuroimaging with a small footprint

With this relatively high amount of computing power in such a physically small size and affordable price, the question is immediate: It is feasible to do neuroimaging on the Pi? The availability of Linux distributions for ARM platforms suggest that yes. However, the binaries for imaging software distributed for popular platforms as x86 (i386) and x86-64 (amd64) cannot work directly. Rather, the applications would need to be compiled from source.

For the FMRIB Software Library (FSL), the source code can be downloaded and the compilation proceed. Much simpler than that, however, is to take a different route: FSL has been included in NeuroDebian. This alone does not seem helpful, as the packages in the repository are only for 32-bit and 64-bit PCs (the i386 and amd64 ports), and SPARC. However, these packages have made into the upstream Debian, which means they are available for all platforms for which Debian itself has been ported. This includes the ARMv7 that powers the Pi, for which the port armhf (for chips that use a hardware floating point unit) can be used.

The steps to have a working installation of FSL on the Pi 2 are described below. Other interesting software, such as FreeSurfer, would need to be compiled from the source. For SPM, there is no Matlab port at the moment, but Octave runs without problems, such that most functionalities are expected to work. Applications based on Java, such as Mango, work without problems.

Requirements

The photo at the top shows the hardware assembly used for this article. The following is required:

  • A Raspberry Pi 2 (Model B).
  • Power source (can be the USB port of another computer).
  • Micro SD card with at least 8 GB (below it is assumed 32 GB).
  • Ethernet cable and a network that provides internet access.
  • Optional: HDMI display and cable, USB keyboard, and possibly a USB mouse if a graphical system will be installed. Alternatively, a headless system also works, with access via SSH. Below it is assumed a display is connected.

The procedure

Step 1: Download the system image kindly prepared by Sjoerd Simons, and uncompress it:

wget https://images.collabora.co.uk/rpi2/jessie-rpi2-20150705.img.gz
gunzip jessie-rpi2-20150705.img.gz

This image contains only a minimal set of Debian Jessie packages. It uses the kernel 3.18.5, and received a few firmware and boot tweaks that are specific to the Pi 2.

Step 2: Use your favourite utility to transfer the image to the micro SD card. For example, using Linux, run the following, replacing /dev/sdX for the letter corresponding to your SD card (warning: this will erase all data stored in the card):

dd bs=1M if=jessie-rpi2-20150705.img of=/dev/sdX

In some systems, the card may be in /dev/mmcblk0 instead in /dev/sdX. If a Linux machine is not available, but instead a Mac or even Windows, the instructions to install Raspbian also apply.

Step 3: Insert the card in the Pi and boot the system. In this image, the default root password is debian (you can change it for something sensible).

Step 4: The main partition in this disk image (mounted as /) has only 2.6 GB, which is not enough. Also, often more than 1 GB of memory is needed, so swap space for virtual memory is necessary. Use fdisk (as root) to expand the main partition and to create a new partition for swap. Usually this is done interactively. If the card has exactly 32 GB, the line below can be used directly, bypassing the interactive mode. It will define a main partition with 24 GB, and the remaining, about 5 GB, will be left for swap. For cards of different sizes, run fdisk manually, or change the line below accordingly.

printf "d\n2\nn\np\n\n\n+24G\nn\np\n\n\n\nt\n3\n82\nw\n" | fdisk -uc /dev/mmcblk0

Note that, when seen from the Pi, the SD card is at /dev/mmcblk0, not /dev/sdX.

Reboot (shutdown -r now), then after logging in again, run:

resize2fs /dev/mmcblk0p2
mkswap /dev/mmcblk0p3
swapon /dev/mmcblk0p3

The swapon command enables the swap partition for immediate use. To make the change permanent for the next reboot, edit the file /etc/fstab adding:

/dev/mmcblk0p3 swap swap defaults 0 0

Step 5: Edit the /etc/apt/sources.list so as to include the official Debian packages (you can replace the server for your favourite/closer mirror):

deb http://ftp.uk.debian.org/debian/ jessie main contrib non-free

Step 6: Refresh the cached list of packages, then install FSL:

apt-get update
apt-get install fsl

Step 7: The installation is almost ready. The downloaded packages do not have the “data” directory of FSL, which contains the atlases and standard space images. To obtain these, do one of the following:

  • From a separate FSL installation (e.g., from a different computer), copy the contents of the ${FSLDIR}/data to the /usr/share/fsl/data of the newly installed system on the Raspberry Pi. This can be done over the network, via ssh, or after plugging in and mounting (with the correct privileges) the card in a different Linux system.
  • If another computer with FSL installed is not available, download FSL for CentOS or Mac (at the end of the downloads page, under “Advanced Users”), then uncompress the downloaded file, and copy the whole contents of the data directory to /usr/share/fsl/data of the Pi via ssh
  • If another computer is not at all accessible for this step, these files can be obtained using the Pi itself, from the command line. Logged in as root in the newly installed system, run:
cd /usr/share
wget -O- http://fsl.fmrib.ox.ac.uk/fsldownloads/fsl-5.0.9-centos6_64.tar.gz | tar xzfv - fsl/data
  • A last option is to skip this step, go to Step 9 below, then download and copy using a graphical web-browser from an installed desktop environment.

Step 8: Add this line to the file ~/.profile:

. /etc/fsl/fsl.sh

That’s it. All that is needed to run FSL from the command line has been done.

Step 9 (optional): The installation up to this step does not include a graphical user interface. To have one, install X and a desktop environment. For lightweight options, LXDE or XFCE can be considered. A screenshot of LXDE with FSLview and two terminal windows showing some system information is below (usually one would not run as root, but create an user account).

Using Raspbian

The official operating system for the Raspberry Pi, Raspbian, is a customised version of Debian, thus capable of running FSL directly. However, FSL is not in the official rpi repository. It can still be installed following similar steps as above, remembering to use sudo with commands require root privileges (the default account is rpi and the password is raspberry), and with care in the repartitioning, as the official disk image uses a different scheme. In Step 5, include the same Debian package source in the /etc/apt/sources.list file.

Overclocking

The Pi can be overclocked. Conservative, stable settings, that do not void the warranty, consist of increasing the CPU frequency to 1000 MHz (from the default 900), the GPU and SDRAM frequencies to 500 MHz (the defaults are 250 and 450 respectively), and the CPU/GPU voltage by 2 steps, i.e., by 2 × 25 mV, from 1.20 to 1.25 V. The overclock settings are adjusted in the file /boot/firmware/config.txt if using Debian (following the steps above), or in /boot/config.txt if using Raspbian:

arm_freq=1000
gpu_freq=500
sdram_freq=500
over_voltage=2

These settings cause the bogomips to jump from 38.40 to 64.00. The temperature of the onboard chips can increase, however, and a suggestion is to use heatsinks or fans, which are inexpensive and can be purchased online (fans would be powered by GPIO pins).

Performance

With the system up and running, it is time for some benchmarks. Although the assembly is exciting and in general the system speed respectable, unfortunately, processing using FEEDS suggests a poor performance. The table below compares the timings of the Pi 2 with default versus overclocked settings, relative to a minimal install of the Debian Jessie on a notebook with an Intel Core i5 processor and 8 GB of RAM.

Default settings Overclocked settings
PRELUDE & FUGUE  6.0  4.8
SUSAN  15.1  11.9
SIENAX  13.3  10.4
BET2  12.3  9.4
FEAT  12.1  9.6
MELODIC  15.9  12.2
FIRST  14.0  11.1
FDT  7.4  5.9
FNIRT  26.6  19.3
Total time  12.2  9.5

Running the whole FEEDS took 22 minutes in the Intel Core i5, whereas in the Pi 2 it took 4h29min with the default settings, and 3h30min after overclocking. It should be noted, however, that the 1 GB of RAM is not sufficient to run the test without using virtual memory (swapping). This needs to be taken into account when evaluating the table above. The SD card used for the tests is a Class 10, which is not as fast as actual RAM (faster cards would have their performance curtailed by hardware limits).

The performances of Debian and Raspbian on the Pi 2 are nearly identical. Running in the graphical mode (at least with LXDE) or in a console-only system do not seem to impact results, at least as far only one instance of FEEDS was running.

Conclusion

It is possible to run FSL on the Raspberry Pi 2, and the procedure is not too different than doing the same in an ordinary computer. The performance, however, suggests that the current model, being about ten times slower, may not be a competitive choice for brain imaging.