similar to: fitting nlme model inside a function

Dear all, I am trying to get a PERMANOVA with quite large data set. I am reading a lot about this question, but I do not get the answer about it. Although I know that the R function is adonis () (vegan package), it does not work: adonis(Pha.env~SPha, data=Pha, permutations=10) The error message: Error: cannot allocate vector of size 334.2 Mb In addition: Warning messages: 1: In vegdist(lhs,

Hi, I am new to R and I am trying to perform a post hoc tukey test using the multcomp package's ghlt for a lme model. My first attempt at doing so gave me an output, HOWEVER I have tried to do this again, it keeps coming up with the error: (Error in contrMat(table(mf[[nm]]), type = types[pm]) : less than two groups) My model is looking at effect of incubation temperature (3 groups) on

Hi Folks - I'm experiencing a very strange problem with Server 2008 machines (for all intents and purposes related to Samba, it's Vista) connecting to a Samba Server. The Samba machine is a RHEL4.6 machine running Samba 3.0.25b. I am joined to the mixed mode AD domain via the command "net rpc join -U administrator <domain>". I am not using winbind or kerberos. Or

On Tue, Mar 6, 2018 at 10:22 PM, Paul Anderson <pha at umich.edu> wrote: > Raghavendra, > > I've commited my tests case to https://github.com/powool/gluster.git - > it's grungy, and a work in progress, but I am happy to take change > suggestions, especially if it will save folks significant time. > > For the rest, I'll reply inline below... > > On Mon,

I suppose that once you've got a 6502 working, adding support for a 4510 shouldn't be too difficult.... (http://c65gs.blogspot.com.au/) On Fri, Jul 4, 2014 at 10:38 AM, Bruce Hoult <bruce at hoult.org> wrote: > On Fri, Jul 4, 2014 at 12:02 PM, Edwin Amsler <edwinguy at gmail.com> wrote: > >> Well, the stack pointer be a single byte, so pushing things on there

On Tue, Mar 6, 2018 at 10:58 PM, Raghavendra Gowdappa <rgowdapp at redhat.com> wrote: > > > On Tue, Mar 6, 2018 at 10:22 PM, Paul Anderson <pha at umich.edu> wrote: > >> Raghavendra, >> >> I've commited my tests case to https://github.com/powool/gluster.git - >> it's grungy, and a work in progress, but I am happy to take change >>

I just modified mail-filter-out.sh like this: cat &nbsp;mail-filter-out.sh &nbsp; #!/bin/sh &nbsp; USER=$1 &nbsp; cat &gt; /tmp/tempfile &nbsp; cat /tmp/tempfile cat &nbsp;/tmp/tempfile This message is in MIME format. --nsmail-7bjyg3nr5o-7bmibqhut9 Content-Type: text/html; charset="UTF-8" Content-Transfer-Encoding: base64

I am having a hard time interpreting the phase and coherency plots. x is two timeseries that occur at the same time i.e. a b 1 11.2 12.3 16 11.3 12.4 31 11.4 12.5 46 11.5 12.6 ...etc even though my example is does not show this they are oscillating at more or less the same frequency just shifted by t=x (imagine two sine waves offset with the 2nd sine

+Csaba. On Tue, Mar 6, 2018 at 2:52 AM, Paul Anderson <pha at umich.edu> wrote: > Raghavendra, > > Thanks very much for your reply. > > I fixed our data corruption problem by disabling the volume > performance.write-behind flag as you suggested, and simultaneously > disabling caching in my client side mount command. > Good to know it worked. Can you give us the

Raghavendra, I've commited my tests case to https://github.com/powool/gluster.git - it's grungy, and a work in progress, but I am happy to take change suggestions, especially if it will save folks significant time. For the rest, I'll reply inline below... On Mon, Mar 5, 2018 at 10:39 PM, Raghavendra Gowdappa <rgowdapp at redhat.com> wrote: > +Csaba. > > On Tue, Mar 6,

Hi, I am an astronomer and somewhat new to boostrap statistics. I understand the basic idea of bootstrap resampling, but am uncertain if it would be useful in my case or not. My problem consists of maximizing a likelihood function based on the velocities of a number of stars. My assumed distribution of velocities of these stars is:

Hi, I tried to Update the Nvidia driver. But the result is a failed because it''s not for Xen Kernel. This the log > [ebuild U ] x11-drivers/nvidia-drivers-270.41.06 [260.19.36] > USE="(multilib) > -acpi -custom-cflags -gtk" 0 kB > > >>> Source > prepared. > >>> Configuring source in >

Hi, I'm using Ubuntu Dapper and I'm trying to emulate GTA San Andreas. Unfortunately, I have ATI Radeon 9600 PRO :( . (I've got the newest drivers 8.26.18) When I'm running Wine, this game starts and works only for a couple of seconds :/ It shows logo of San Andreas, and after that it crashes. Wine shows this bug: fixme:system:SystemParametersInfoW Unimplemented action: 8193

On Mon, Mar 5, 2018 at 8:21 PM, Paul Anderson <pha at umich.edu> wrote: > Hi, > > tl;dr summary of below: flock() works, but what does it take to make > sync()/fsync() work in a 3 node GFS cluster? > > I am under the impression that POSIX flock, POSIX > fcntl(F_SETLK/F_GETLK,...), and POSIX read/write/sync/fsync are all > supported in cluster operations, such that in

# gluster --version glusterfs 3.3.1 built on Oct 11 2012 22:01:05 # gluster volume info Volume Name: gdata Type: Distribute Volume ID: eccc3a90-212d-4563-ae8d-10a77758738d Status: Started Number of Bricks: 3 Transport-type: tcp Bricks: Brick1: gluster-0-0:/mseas-data-0-0 Brick2: gluster-0-1:/mseas-data-0-1 Brick3: gluster-data:/data [root at mseas-data ~]# ps -ef | grep gluster root 2783

Raghavendra, Thanks very much for your reply. I fixed our data corruption problem by disabling the volume performance.write-behind flag as you suggested, and simultaneously disabling caching in my client side mount command. In very modest testing, the flock() case appears to me to work well - before it would corrupt the db within a few transactions. Testing using built in sqlite3 locks is

Well, the stack pointer be a single byte, so pushing things on there doesn't work terribly well. Assuming I pass by reference, that's 128 values absolutely total before it wraps around and silently clobbers itself. It means single byte values will be incredibly inefficient... Tricky stuff. I'm lucky on the C64 since it's rare to exit back to the kernel with machine language apps

Hello, On Thursday, September 20, 2018 11:15:04 AM EDT Duncan Murdoch wrote: > On 20/09/2018 6:59 AM, Ralf Stubner wrote: > > On 9/20/18 1:43 AM, Carl Boettiger wrote: > >> For a well-tested C algorithm, based on my reading of Lemire, the > >> unbiased "algorithm 3" in https://arxiv.org/abs/1805.10941 is part > >> already of the C standard library in

On CentOS5 with the latest updates applied, the logwatch filter for postfix returns way too many lines from the log. I get an "unmatched entries" message and all messages that have gone through the system is listed. Here is an example: 8F930A8092: to=<morten at foo.bar>, orig_to=<morten at localhost>, relay=local, delay=0.19, delays=0.06/0.01/0/0.12, dsn=2.0.0,

Hi, tl;dr summary of below: flock() works, but what does it take to make sync()/fsync() work in a 3 node GFS cluster? I am under the impression that POSIX flock, POSIX fcntl(F_SETLK/F_GETLK,...), and POSIX read/write/sync/fsync are all supported in cluster operations, such that in theory, SQLite3 should be able to atomically lock the file (or a subset of page), modify pages, flush the pages to