If
you know exactly what you are going to do, what is the point of doing
it? Pablo
Picasso Every line in your calculations ends with "=0". You are not making much progress! Kate Hammett We don't do the calculation because we don't know the answer, we do it because we have a conscience. Bryan Taylor Let's change the resolution on the Unknown. Gabe Plunk Let me put it differently: suppose we had a reactor... Per Helander Working together takes more than one person. Bill Dorland We can't do ultraviolence to that square bracket. Ian Abel Field lines are forever. Bryan Taylor This is not really an ill-posed problem, this is not a problem at all. Paul Dellar I am just doing mathematics at the moment, but it is mathematics that has some point. Bryan Taylor The equivalent of God in MAST is MHD, which is global and all powerful. Anthony Field I've got a fishbone coming up. Tim Horbury We have crossed all the i's and dotted all the t's. Job's a good'un. Ian Abel Let us not jump in front of the bandwagon! Anonymous It's not the triviality, it's the emptiness of it that bothers me. Bryan Taylor | It is
better to be roughly right than precisely wrong. Maynard
Keynes This is a very inefficient way of achieving nothing. François Rincon We Hankel all the way in and then Hankel all the way out. Joseph Parker For the sake of fairness, let me mention that some people have objections to this, none of which are particularly valid. Chris Chen Yes, Steve, you have always known what we have only just figured out. Alfred Mallet This is more or less right. Perhaps less. Alfred Mallet You go ahead with your argument. I'll think. Steve Cowley Too simple? At the end of my talk, you will beg for simplicity! Andrey Beresnyak The point is not the point! Anonymous This is why I am presenting this here and nowhere else: nothing is solved! Ian Abel This calculation is not intellectual masturbation: there's no orgasm. Anonymous There are many big Buts here... I like big Buts. Anonymous Previous studies of this problem have been either unsatisfactory or limited in scope.---What is the difference between these?---This means either wrong or irrelevant. Anatoly Spitkovsky, Michael Medvedev and Steve Cowley (in conversation) I don't give a damn about astrophysics, explain to me what is going on. Anatoly Spitkovsky |
Wk | Date |
Time & place |
Speaker & Topic |
Background reading |
Comings and goings (incl. visitors in town) |
Thu 1 Sept |
11:30 Fisher Rm |
Plasma
Group Meeting (organised
by MICHAEL) Group discussion. New arrivals: Yohei Kazwazura and Adwiteey Mauriya (see Background Reading if you want to read up on their past research). |
arXiv:1602.01165 PoP 22, 112503 (2015) J. Phys. A 47, 465501 (2014) PoP 19, 082513 (2012) PoP 19, 012305 (2012) PRE 82, 066403 (2010) ApJ 790, 125 (2014) |
Yohei Kawazura joins the group as STFC PDRA Adwiteey Mauriya (IST, Lisbon) joins the group as a visiting student (with M. Barnes & F. Nave) Nicolas Christen joins the group as DPhil student (to work with M. Marnes) |
|
Mon 5 Sept |
11:30 501 DWB |
Plasma
Seminar (organised by ALEX) Eugene Churazov (MPA Garching) --- (1) Update on Hitomi results on galaxy-cluster turbulence and their physics implications (2) Not that long time ago in the nearest galaxy: 3D slice of molecular gas revealed by a 110 years old flare of Sgr A* (and a programme for the next few hundred years of X-ray observations of our Galaxy) |
(1) Nature 535,
117 (2016) (2) preprint from author on request |
Eugene
Churazov (MPA Garching) |
|
Thu 15 Sept |
11:30 501 DWB |
Plasma
Group Meeting (organised
by MICHAEL) Summer projects update: Paolo Abiuso & Michael Barnes --- Pair plasmas heating |
Paolo
Abiuso (SNS) finishes his summer internship with M. Barnes |
||
Thu 22 Sept |
11:30 501 DWB |
Plasma Seminar (organised
by ALEX) Yohei Kawazura (Tokyo--->Oxford) --- Particle acceleration in a laboratory magnetosphere |
arXiv:1602.01165 PoP 22, 112503 (2015) a version of slides |
Jason
Parisi and Valerian Chen join the group as DPhil students (to work with F. Parra) |
|
26-30 Sept |
Gyrokinetic Theory Working Group Meeting
in Madrid |
||||
Thu 29 Sept |
No seminar |
||||
0 |
Thu Oct 6 |
11:30 501 DWB |
Plasma Seminar (organised
by MICHAEL) Yohei Kawazura (Tokyo--->Oxford) --- Action principle for relativistic extended magnetohydrodynamics |
arXiv:1611.06036 |
Plamen
Ivanov joins the group as DPhil student (to work with A. Schekochihin) |
I |
Thu Oct 13 |
11:30 501 DWB |
Plasma
Seminar (organised by
ALEX) Romain Meyrand (SSL Berkeley & LPP Paris) --- Waves and turbulence in magneto-fluid |
JFM 770, R1 (2015) PRL 116, 105002 (2016) |
Romain Meyrand (SSL, Berkeley) |
Fri 14 Oct |
14:00 rm 277 7 Keble Rd |
Oxford e-Research Centre Seminar: Colin Roach (CCFE) --- Fusion, plasma turbulence and computational challenge |
|||
II |
Thu Oct 20 |
11:30 501 DWB |
Plasma
Group Meeting (organised
by MICHAEL) Michael Barnes --- Tutorial lecture: Overview of tokamak transport and scaling laws for tokamak turbulence This a crash course aimed especially at graduate students. The following reading is recommended: 1) Students should be familiar with random walks and diffusion; if you are not please educate yourselves 2) Multiscale GK theory: a comprehensive review is Abel et al. (2013) Rep. Prog. Phys. 76, 116201 (you're not expected to read this fully before the lecture, but do take a look); see also PPCF 50, 065014 (2008) for another now classic treatment; the baby version of GK (slab) very good for initial learning: ApJ 651, 590 (2006) 3) Multiscale GK numerics: PoP 17, 056109 (2010) 4) Critical balance in fusion context: PRL 107, 115103 (2011) 5) Scaling laws for turbulent heating: PRL 109, 185003 (2012) |
look on the right Michael's slides (pptx) |
|
III |
Thu Oct 27 |
11:30 501 DWB |
Plasma
Group Meeting (organised
by ALEX) Alex Schekochihin --- Update on MAST turbulence: subcritical transition, electron collisionality scaling/zonal flows, etc. (based on the theses of G. Colyer, F. van Wyk & M. Fox) |
arXiv:1607.06752 arXiv:1607.08173 arXiv:1609.08981 another preprint on request from F. van Wyk |
Ian Abel (Chalmers) G. Ravindra Kumar (Tata Inst.) Alfred Mallet (UNH) Anvar Shukurov (Newcastle) Michael Fox |
Fri Oct 28 |
15:30 501 DWB |
Plasma Seminar (organised
by GIANLUCA & ALEX) G. Ravindra Kumar (Tata Institute) --- Ultrafast plasma dynamics and giant magnetic fields in intense laser-matter interactions High
intensity, ultrashort light pulses (>10^18 W/cm^2, femtosecond
duration) are revolutionising science and technology in very exciting
ways, whether it is laboratory simulation of astrophysical phenomena,
relativistic optics, table-top particle acceleration, real-time X-ray
diffraction of the condensed phase or medical therapies for cancer. All
these phenomena rely crucially on the generation and transport of
relativistic electrons in a target. This talk will present studies of
the transport of the mega-ampere current of these electrons through
dense matter, using ultrafast pump-probe experiments. We will look at
the evolution of multi-megagauss magnetic pulses at femtosecond
temporal and micron spatial resolution in the plasma [1, 2]. We will
examine the electron filamentation process and the turbulent behavior
of the magnetic field [1, to be published]. Similarities between our
results and astrophysical observations indicate the rich scope offered
by table top terawatt lasers for pursuing laboratory astrophysics. We
will also touch upon our studies on the ultrafast dynamics of
femtosecond laser generated plasma involving Doppler spectrometry [3]
and Cherenkov emission.
|
[1] PNAS 109, 8011 (2012) [2] PRL 108, 235005 (2012) [3] PRL 114, 115001 (2015) |
||
IV |
Thu Nov 3 |
11:30 501 DWB |
Plasma Seminar (organised
by ALEX) Andrey Beresnyak (NRL) --- Charged particles in turbulence Most astrophysical
objects are sources of non-thermal emission produced by energetic
particles. Particles may be accelerated in shocks or current layers or
just in turbulence. Even in shocks, which are very efficient
accelerators, interaction with turbulence is critical because particles
must scatter through self-generated turbulence. Speaking of turbulence,
a common way to look at it as an agent that facilitates diffusion and
mixing. I will show, however, that turbulence can un-mix particles,
creating free energy in the initial equilibrium distribution. This
curious property depends only on the geometry of the magnetic field
lines, e.g. field lines can act as a Maxwellian demon for particles
[1]. Likewise, turbulence had been imagined as a completely random
process in which particles can only be accelerated by the slow
second-order process. In fact, recently we found a surprising
analytical connection between first order acceleration rate and a
certain statistical property of turbulence which is often non-zero [2].
In other words, turbulence is not random and it can, volumetrically,
accelerate or decelerate particles in the first order process.
|
[1] ApJ 767, 39L (2013) [2] ApJ 819, 90 (2016) |
Andrey Beresnyak (NRL) Adwiteey Mauriya returns to Lisbon |
V |
Thu Nov 10 |
11:30 501 DWB |
Plasma
Group Meeting (organised
by ALEX) Felix Parra --- Stellarators close to omnigeneity Extended reading list: Phys. Fluids B 3, 2822 (1991) PRL 78, 674 (1997) PoP 4, 3323 (1997) Nucl. Fusion 55, 033005 (2015) arXiv:1610.06016 |
PoP 19, 056103 (2012) ++extended reading list (look on the right) |
Ian Abel (Chalmers) Felix Parra comes back from his sabbatical in Spain |
VI |
Thu Nov 17. |
11:30 501 DWB |
Plasma Seminar (organised
by MICHAEL) Greg Hammett (Princeton) --- Full-f gyrokinetic simulations of the LAPD device with open field lines and sheath boundary conditions |
arXiv:1610.09056 |
Greg Hammett (Princeton) Ian Abel (Chalmers) |
VII |
Thu Nov 24. |
11:30 501 DWB |
Plasma
Group Meeting (organised
by MICHAEL) Free discussion/research updates |
Michael Fox (St Olave's) |
|
VIII |
Thu Dec 1. |
11:30 Fisher Rm |
Plasma Seminar (organised
by MICHAEL) William Bethune (Grenoble) --- Non-ideal magnetohydrodynamics in protoplanetary disks |
arXiv:1603.02475 +preprint from speaker on request |
William Bethune (Grenoble) |
9 |
Thu Dec 8 |
11:30 501 DWB |
Plasma Seminar (organised
by ALEX) Troy Carter (UCLA) --- Electromagnetic turbulence and transport in increased-beta LAPD plasmas |
RSI 87, 025105 (2016) PoP 22, 062105 (2015) +2 preprints from speaker on request |
Troy Carter (UCLA) Nuno Loureiro (MIT) Scott Melville (Imperial) |
10 |
Thu Dec 15 |
11:30 501 DWB |
Plasma
Group Meeting (organised
by ALEX) Updates from everyone |
Antoine Bret (U. Castilla La Mancha) |
|
Thu Dec 22 |
No seminar. Merry Xmas! |
||||
Thu Dec 29 |
No seminar. Happy NY! |