Author Archive

Go Galaxy!

Posted in Uncategorized with tags on August 5, 2009 by telescoper

This morning I was looking through my copy of the popular monthly periodical British Naturism (which I buy for the Spot-the-Ball competition).

In the magazine I found an advertisement with the slogan

If you can’t go naked, go Galaxy!

The immediate thing that sprang to mind was that I didn’t think I’d ever seen Galaxy used as an adjective before. However, this is advertising so the usual rules of grammar don’t apply. The next question was whether it might have something to do with astronomy. It doesn’t.

Galaxy is the strangest range of clothing you’ve ever seen. Essentially it contains bathing costumes that are almost transparent, enabling the Sun’s rays to pass through the material. At the same time a kind of disruptive pattern camouflage (available in a choice of designs) printed on the meshlike material makes the items appear opaque to prying eyes. Here’s an example

shortnn

This combination allows the wearer to acquire a suntan in his or her private places but the swirling patterns confuse the observer’s eye to the extent that he/she doesn’t realise that the wearer’s personal credentials are actually in full view. Perhaps this is an example of Moiré is less?

Having been swimming au naturel on many occasions, I would say the best part of it is the freedom you feel in having your private parts unconstrained. The downside is the exposure of sensitive areas to the harsh rays of the Sun. It seems to me that in this sense the Galaxy range offers the worst possible combination of being hindered as well as burnt. Still, they do offer an option to those people who are too shy to go nude on a beach and who want to get an all over tan without using one of those horrendous ultra-violet tanning machines that look like a fluorescent coffin or slapping  orange dye all over themselves.

I’m not sure how effective these things are at concealing the relevant appendages, so maybe I’ll buy a pair and see. Perhaps I could run an undergraduate project to investigate their optical properties?

Singh Along

Posted in Science Politics with tags , , , on August 4, 2009 by telescoper

One of the nice things about the blog interface at  WordPress  is the way it flags up posts from other blogs that might be related to those on your own site. A good example is an item at a site which is quite new to me called Cubik’s Rube. This particular one alerted me to an update about the Simon Singh libel action which I’ve blogged about before, in a post that generated a great deal of debate and discussion.

If you recall, Singh is being sued for libel by the British Chiropractic Association (BCA)  for damages after he labelled some of their treatments bogus in an article written in The Guardian. The newspaper settled and withdrew the piece from its website but Singh decided to fight the action. At a pre-trial hearing the judge ruled that his use of the word bogus would be interpreted as meaning that the therapies being offered by the BCA were not only worthless, but that the BCA  knew they were worthless. To win his case Singh would have to prove both these claims were true. Simon Singh claimed he never intended that meaning and vowed to appeal. That was the situation in June 2009, at the time of my previous post.

Things moved on a bit while I was away last week. In an order sealed on 30 July 2009 the Court of Appeal has refused Singh leave to appeal, thus piling the pressure even further on him to settle the action and restricting his options even further. For a clearer explanation of the legal issues involved than I could ever manage, see the article by famous legal blogger Jack of Kent.

One side issue is worth mentioning, however, which is that it is apparently unclear from a legal point of view whether the BCA has standing to sue for defamation at all since it is a corporation without shareholders. It seems strange that such a basic issue would be unresolved. Surely there must be relevant precedents?

Meanwhile the BCA has issued a conciliatory statement, implying that it would prefer for the case to be settled out of court. This seems a bit surprising given that they would appear to hold all the cards, but the answer probably lies in the appalling public relations gaffe it has made over its presentation of alleged evidence for its therapies.

Challenged (largely by bloggers) to present evidence for the effectiveness of its therapies for certain paediatric conditions (such as asthma, infantile colic and even bed-wetting), the BCA produced a report containing a “plethora” of evidence, dated 17th June 2009. This dossier – cobbled together from 19 research papers, most of which don’t really support their case at all – turns out to have been the epitome of dodginess and over the last few weeks it has been comprehensively dissected, discredited, debunked and demolished all over the blogosphere. A recent editorial in the British Medical Journal described its own refutation of the BCA’s claims to be “complete”.

I doubt if the BCA wants to see its credibility further undermined by having its so-called evidence savaged again in open court, which probably explains why they might prefer to settle than carry on the case. Nothing said in court can be subject to the libel laws.

But it’s an amazing blunder by the BCA to have presented such a shaky collection of evidence in the first place. All it has achieved is to make them look like fools.

Anyway, it’s now a peculiar situation. It still looks like Singh can’t win the case unless he can prove the BCA are dishonest rather than merely inept. And the BCA stands to fall even lower in public esteem if it goes to trial. If Singh can afford it he could fight on regardless and hope that if he loses the damages will be bearable. Morally, though, he will have won.

But the really impressive thing to me is the way that expert bloggers have forced the BCA into a corner. I think this is probably a sign of the way science is changing through use of the internet’s ability to communicate complex things so rapidly.

Return of the Clerihews!

Posted in Poetry, The Universe and Stuff with tags , , on August 2, 2009 by telescoper

As a result of an after-dinner discussion at the meeting I attended last week, I’ve decided to put a revised cosmological clerihew collection back online. I’ve removed or edited those that caused the greatest offence, and added a few new ones.

Bernard Carr
Has gone a bit far:
His Anthropic Principle
Makes theories invincible

Sean Carroll
Has me over a barrel
Because the only plausible rhyme
Plugs his new book on Time

The mind of John Barrow
Is not very narrow:
He’s more open than me
To a variable c

Stephen Hawking
Lets a machine do the talking
But even  he can’t vocalize in-
side a black hole horizon.

Joe Silk
Is one of that ilk
Who writes far more articles
Than there are elementary particles

Matt Griffin
Has healthy salad for tiffin
But he’d probably expire
If something went wrong with SPIRE.

Peter Ade
Would never be afraid
To enter his name
In the citation game

Andy Lawrence
Would shed tears in torrents
If they finally got rid
Of the Astrogrid

Steve Maddox
Never eats haddocks
But he’s quite a dab hand
In the optical band

Ofer Lahav
Is awfully suave
But must be getting nervy
About the cancellation of funding for the Dark Energy Survey

Joao Magueijo
Was on the Today Show
Talking some shite
About travelling faster than light

Keith Mason
Said to Lord Drayson
“Can we have some more money?”
He replied “Don’t try to be funny…”

Andrei Linde
Felt rather windy
A peculiar sensation:
The result of internal inflation?

To rhyme Carlos Frenck
I’ve drawn a complete blenk
But I found in the lexicon
A good one for Mexican

When Andrew Jaffe
Plots a new graph he
Thinks fits his theory he’ll
Tell everyone at Imperial

Paul Steinhardt
Said “Lust not after beauty in thine heart”
But why he did so
I really don’t know

Feel free to offer your own through the comments box, after consulting the rules, although I remind you I don’t accept anonymous comments, even if they’re funny.

The End of All Songs

Posted in Music with tags , , on August 1, 2009 by telescoper

I’ve been searching around on Youtube for quite a while trying to decide which is my favourite version of my favourite song. This is Im Abendrot, a poem by Joseph von Eichendorff, as it was set to music by Richard Strauss and published as the last of his Four Last Songs. Strauss wrote the music for this in 1948, just a year before he died.

The poem had a special meaning for Strauss and I think that comes across in the achingly beautiful music he composed for it. The verse is

Wir sind durch Not und Freude
gegangen Hand in Hand;
vom Wandern ruhen wir
nun überm stillen Land.

Rings sich die Täler neigen,
es dunkelt schon die Luft,
zwei Lerchen nur noch steigen
nachträumend in den Duft.

Tritt her und laß sie schwirren,
bald ist es Schlafenszeit,
daß wir uns nicht verirren
In dieser Einsamkeit.

O weiter, stiller Friede!
So tief im Abendrot.
Wie sind wir wandermüde–
Ist dies etwa der Tod?

Although it is basically about death, I find this piece immensely uplifting and joyful.  The setting of the last verse in particular reaches parts of me that other music doesn’t reach. The voice floats freely as if suspended in mid-air over the first line (O weiter, stiller Friede!) while the orchestra gently swells beneath it, heightening the suspense. The voice then soars up and away like a majestic bird over the second line of text (So tief im Abendrot) while the orchestra gathers again. The exquisite countermelody rises up to meet the vocal line and they fly together for a while before the words come to and end and it all eventually subsides into a quiet but wonderful sense of fulfilment and peace.

Music just doesn’t get much better than this.

This is the best version I could find on Youtube, by the relatively unknown Gundula Janowitz recorded in 1973 with the Berlin Philharmonic. I’m not saying it’s the best version that’s ever been done – this piece has been recorded by virtually every soprano worthy of the name and everyone will have their favourite- but this is up among the very best.

A Mountain of Truth

Posted in Bad Statistics, The Universe and Stuff with tags , , , , on August 1, 2009 by telescoper

I spent the last week at a conference in a beautiful setting amidst the hills overlooking the small town of Ascona by Lake Maggiore in the canton of Ticino, the Italian-speaking part of Switzerland. To be more precise we were located in a conference centre called the Centro Stefano Franscini on  Monte Verità. The meeting was COSMOSTATS which aimed

… to bring together world-class leading figures in cosmology and particle physics, as well as renowned statisticians, in order to exchange knowledge and experience in dealing with large and complex data sets, and to meet the challenge of upcoming large cosmological surveys.

Although I didn’t know much about the location beforehand it turns out to have an extremely interesting history, going back about a hundred years. The first people to settle there, around the end of the 19th Century,  were anarchists who had sought refuge there during times of political upheaval. The Locarno region had long been a popular place for people with “alternative” lifestyles. Monte Verità (“The Mountain of Truth”) was eventually bought by Henri Oedenkoven, the son of a rich industrialist, and he  set up a sort of commune there at  which the residents practised vegetarianism, naturism, free love  and other forms of behaviour that were intended as a reaction against the scientific and technological progress of the time.  From about 1904 onward the centre became a sanatorium where the discipline of psychoanalysis flourished and it later attracted many artists. In 1927,   Baron Eduard Von dey Heydt took the place over. He was a great connoisseur of Oriental philosophy and art collector and he established  a large collection at Monte Verità, much of which is still there because when the Baron died in 1956 he left Monte Verità to the local Canton.

Given the bizarre collection of anarchists, naturists, theosophists (and even vegetarians) that used to live in Monte Verità, it is by no means out of keeping with the tradition that it should eventually play host to a conference of cosmologists and statisticians.

The  conference itself was interesting, and I was lucky enough to get to chair a session with three particularly interesting talks in it. In general, though, these dialogues between statisticians and physicists don’t seem to be as productive as one might have hoped. I’ve been to a few now, and although there’s a lot of enjoyable polemic they don’t work too well at changing anyone’s opinion or providing new insights.

We may now have mountains of new data in cosmology in particle physics but that hasn’t always translated into a corresponding mountain of truth. Intervening between our theories and observations lies the vexed question of how best to analyse the data and what the results actually mean. As always, lurking in the background, was the long-running conflict between adherents of the Bayesian and frequentist interpretations of probability. It appears that cosmologists -at least those represented at this meeting – tend to be Bayesian while particle physicists are almost exclusively frequentist. I’ll refrain from commenting on what this might mean. However, I was perplexed by various comments made during the conference about the issue of coverage. which is discussed rather nicely in some detail here. To me the question of of whether a Bayesian method has good frequentist coverage properties  is completely irrelevant. Bayesian methods ask different questions (actually, ones to which scientists want to know the answer) so it is not surprising that they give different answers. Measuring a Bayesian method according to  a frequentist criterion is completely pointless whichever camp you belong to.

The irrelevance of coverage was one thing that the previous residents knew better than some of the conference guests:

mvtanz3

I’d like to thank  Uros Seljak, Roberto Trotta and Martin Kunz for organizing the meeting in such a  picturesque and intriguing place.

Beautiful Cosmos

Posted in Poetry with tags , on July 26, 2009 by telescoper

I’m currently in transit to a conference in Ascona (Switzerland) so I thought I’d leave you for a while with something from the wacky and whimsical, weird and wonderful world of Ivor Cutler:

Astronomy or Astrophysics?

Posted in The Universe and Stuff with tags , , , , , on July 25, 2009 by telescoper

A chance encounter with the parent of a prospective student the other day led eventually to the question What’s the difference between Astronomy and Astrophysics? This is something I’m asked quite often so I thought I’d comment on here for those who might stumble across it. I teach a first-year course module entitled “Astrophysical Concepts”. One of the things I try to do in the first lecture is explain that difference. The Oxford English Dictionary gives the following primary definition for astronomy:

The science which treats of the constitution, relative positions, and motions of the heavenly bodies; that is, of all the bodies in the material universe outside of the earth, as well as of the earth itself in its relations to them.

Astrophysics, on the other hand, is described as

That branch of astronomy which treats of the physical or chemical properties of the celestial bodies.

So astrophysics is regarded as a subset of astronomy which is primarily concerned with understanding the properties of stars and galaxies, rather than just measuring their positions and motions. It is possible to assign a fairly precise date when astrophysics first came into use in English because, at least in the early years of the subject, it was almost exclusively associated with astronomical spectroscopy. Indeed the OED gives the following text as the first occurence of astrophysics, in 1869:

As a subject for the investigations of the astro-physicist, the examination of the luminous spectras of the heavenly bodies has proved a remarkably fruitful one

The scientific analysis of astronomical spectra began with a paper  William Hyde Wollaston in the Philosophical Transactions of the Royal Society Vol. 102, p. 378, 1802. He was the first person to notice the presence of dark bands in the optical spectrum of the Sun. These bands were subsequently analysed in great detail by Joseph von Fraunhofer in a paper published in 1814 and are now usually known as Fraunhofer lines.  Technical difficulties  made it impossible to obtain spectra of stars other than the Sun for a considerable time, but  William Huggins finally succeeded in 1864. A drawing of his pioneering spectroscope is shown below.

Meanwhile, fundamental work by Gustav Kirchoff and Robert Bunsen had been helping  to establish an understanding the spectra produced by hot gases.  The identification of features in the Sun’s spectrum  with similar lines produced in laboratory experiments led to a breakthrough in our understanding of the Universe whose importance shouldn’t be underestimated. The Sun and stars were inaccessible to direct experimental test during the 19th Century (as they are now). But spectroscopy now made it possible to gather evidence about their chemical composition as well as physical properties. Most importantly, spectroscopy provided definitive evidence that the Sun wasn’t made of some kind of exotic unknowable celestial material, but of the same kind of stuff (mainly Hydrogen) that could be studied on Earth.  This realization opened the possibility of applying the physical understanding gained from small-scale experiments to the largest scale phenomena that could be seen. The science of astrophysics was born. One of the leading journals in which professional astronomers and astrophysicists publish their research is called the Astrophysical Journal, which was founded in 1895 and is still going strong. The central importance of the (still) young field of spectroscopy can be appreciated from the subtitle given to the journal: Initially the branch of physics most important to astrophysics was atomic physics since the lines in optical spectra are produced by electrons jumping between different atomic energy levels. Spectroscopy of course remains a key weapon in the astrophysicist’s arsenal but nowadays the term is taken to mean any application of physical laws to astronomical objects. Over the years, astrophysics has gradually incorporated nuclear and particle physics as well as thermodynamics, relativity and just about every other branch of physics you can think of. I realise, however, that this  isn’t really the answer to the question that potential students want to ask. What they (probably) want to know is what is the difference between undergraduate courses called Astronomy and those called Astrophysics? The answer to this one depends very much on where you want to study. Generally speaking the differences are in fact quite minimal. You probably do a bit more theory in an Astrophysics course than an Astronomy course, for example. Your final-year project might have to be observational or instrumental if you do Astronomy, but might be theoretical in Astrophysics.  If you compare the complete list of modules to be taken, however, the difference will be very small.

Over the last twenty years or so, most Physics departments in the United Kingdom have acquired some form of research group in astronomy or astrophysics and have started to offer undergraduate degrees with some astronomical or astrophysical content. My only advice to prospective students wanting to find which course is for them is to look at the list of modules and projects likely to be offered. You’re unlikely to find the name of the course itself to be very helpful in making a choice. One of the things that drew me into astrophysics as a discipline (my current position is Professor of Theoretical Astrophysics) is that it involves such a wide range of techniques and applications, putting apparently esoteric things together in interesting ways to develop a theoretical understanding of a complicated phenomenon. I only had a very limited opportunity to study astrophysics during my first degree as I specialised in Theoretical Physics.  This wasn’t just a feature of Cambridge. The attitude in most Universities in those days was that you had to learn all the physics before applying it to astronomy. Over the years this has changed, and most departments offer some astronomy right from Year 1. I think this change has been for the better because I think the astronomical setting provides a very exciting context to learn physics. If you want to understand, say, the structure of the Sun you have to include atomic physics, nuclear physics, gravity, thermodynamics, radiative transfer and hydrostatics all at the same time. This sort of thing makes astrophysics a good subject for developing synthetic skills while more traditional physics teaching focusses almost exclusively on analytical skills. Indeed, my first-year Astrophysical Concepts course is really a course about modelling and problem-solving in physics.

Going Forward

Posted in Uncategorized with tags , , , on July 22, 2009 by telescoper

Since I’ve recently been officially awarded the title of Grumpy Old Man, I now feel I have the necessary authorization to vent my spleen about anything and everything that really irritates me.

This morning I got my regular monthly credit card statement, something likely to put me in a bad mood at the best of times. However, at the end of the itemized list of payments, I found the following:

WE ARE PHASING OUT CREDIT CARD CHEQUES. GOING FORWARD WE WILL NO LONGER ISSUE ANY CREDIT CARD CHEQUES.

I don’t actually care about the credit card cheques – they’re a ridiculously bad way of paying for things anyway –  but what on Earth is the phrase going forward doing in that sentence?

I’ve taken a swipe at this monster once before, when I blogged about the Wakeham Review of Physics. The example I found then was

The STFC’s governance structure must be representative of the community it serves in order to gain stakeholders’ confidence going forward.

Aaargggh!!

Going forward is one of those intensely annoying bits of office-speak that have spread like Swine ‘flu into the public domain. Pushing the envelope is another one. What does it mean?  Why would anyone push an envelope?

Anyway, the worst problem with going forward is that it is now used almost universally in official documents instead of more suitable phrases, such as in future, or from now on. What particularly irritates me about it is that it is usually part of an attempt to present things in a positive light even when they clearly don’t involve any forward movement at all; often, in fact, quite the opposite. It is just one symptom of the insidious culture of spin that seems to be engulfing all aspects of public life, making it impossible to deliver even a simple message without wrapping it up in some pathetic bit of PR. Any kind of change – whether or not there’s any reason for it, and whether or not it improves anything – has to be portrayed as progress. It drives me nuts!

This sort of language is frequently lampooned by Laurie Taylor in his brilliant weekly column for the Times Higher.  The Director of Corporate Affairs for the fictional Poppleton University, Mr Jamie Targett, contributes regularly to his column, always in meaningless business-oriented gibberish of this type. In fact, shortly after reading the Wakeham Review quoted above, I sent a letter to the Times Higher (which was published there) accusing Jamie Targett of moonlighting from his job at Poppleton to work on the Wakeham Report.

In the case of my credit card cheques, the implication is that the withdrawal of the service represents some sort of progress. In fact, it’s just to save money. A friend of mine who uses a local gym told me today that the gym had recently announced that

Going forward, members of the gym will no longer be supplied with free towels.

They went on to portray this as a great leap forward in caring for the environment, but in fact it is obviously just a way of saving their costs. Likewise with a sentence I found in a railway timetable recently:

Going forward the 8.15 train from Paddington will no longer call at Didcot Parkway

At least it’s still going to call at Didcot when it’s going backwards, which is the obvious implication of this sentence.

I’m glad I’m not alone in my disapproval of going forward.  A year or so ago there was an article on the BBC website making much the same point. However, the amount of going forward has continued to increase. Robert Peston, the BBC business editor, once managed three going forwards in a four minute item on the Today programme.

The Science and Technology Facilities Council has obviously taken this phrase to heart. Their website is chock-a-block with going forward. Here’s an example (referring to a budget cut)

It will result in an approximately constant volume of project activity going forward ..

Obviously, once you start going forward there’s no going back, even if what lies in front of you is financial catastrophe…

PS. Feel free to add your own pet hates via the comments box going forward.

Cricketing Clerihews

Posted in Cricket with tags on July 22, 2009 by telescoper

Undaunted by the ructions caused by my previous attempt (now removed) to have a bit of fun by posting a few clerihews, I’ve decided to try again but this time the target is cricketers.

Please keep them polite, unless they’re about Australians. Bonus points to anyone who manages one about Ben Hilfenhaus. Here are a few to get you started:

If you see Nathan Hauritz
Starting to glower, it’s
Because a humdinger
Hit his right index finger

Andrew Flintoff
Was man-of-the-match by dint of
Some excellent bowling
Well worth extolling

Peter Siddle
Went for a piddle
And when he came back
He’d quite lost the knack

Alastair Cook
Likes to go for the hook
But when it’s more full
He goes for the pull

Andrew Strauss
May have raised a few doubts:
It was well worth a shout
But should have been “not out”..

Michael Clarke
Batted well in the dark
But looked like a chump
When he lost his off stump

Michael Hussey
Is not very fussy
Whether he edges or nicks
Or just wallops for six

Philip Hughes
Can never refuse
An offside dab
That the slips might just grab

Marcus North
Bravely marched forth
To face the England attack
But very soon marched back

Graham Onions
Bowls like he has bunions
But let there be – please –
A bowler called Cheese

In a Galaxy, Faraday…

Posted in The Universe and Stuff with tags , , , , on July 21, 2009 by telescoper

I was finishing off the draft of a paper the other day and remembered a little paper I did some time ago with a former PhD student of mine, Patrick Dineen. I thought it would be fun to put the pictures up here because it was one of those occasions when a little idea turns out much nicer than you expected…

What we had to start with was a collection of Faraday Rotation measurements of extragalactic radio sources dotted around the sky. Their distribution is fairly uniform but I hasten to add that it was not a controlled sample so it would be not possible to take the sources as representative of anything for statistical purposes.

Faraday rotation occurs because left and right-handed polarizations of electromagnetic radiation travel at different speeds along a magnetic field line. The effect of this is for the polarization vector to be rotated as light waves travel and the net rotation angle (which can be either positive or negative) is related to the line integral of the component of the magnetic field along the line of sight travelled by the waves. The picture below shows the distribution of sources, plotted in Galactic coordinates and coded black for negative and white for positive.

rotation

Some radio galaxies have enormously large Faraday rotation measures because light reaches us through regions of the source that have strong magnetic fields. However, for most sources in our sample the rotation measures are smaller and are thought to be determined largely by the propagation of light not through the emitting galaxy, near the start of its journey towards us, but through our own Galaxy, the Milky Way, which is near the end of its path.

If this is true then the distribution of rotation measures across the sky should contain information about the magnetic field distribution inside our own Galaxy. Looking at the above picture doesn’t give much of a hint of what this structure might be, however.

What Patrick and I decided to do was to try to make a map of the rotation measure distribution across the sky based only on the information given at the positions where we had radio sources. This is like looking at the sky through a mask full of little holes at the source positions. Using a nifty (but actually rather simple) trick of decomposing into spherical harmonics and transforming to a new set of functions that are orthogonal on the masked sky we obtained the following map:

uni_16_rmjoint

(The technical details are in the paper, if you’re interested.) You probably think it looks a bit ropey but, as far as I’m concerned, this turned out stunningly well. The most obvious features are a big blue blob to the left and a big red blob to the right, both in the Galactic plane. What you’re seeing in those regions is almost certainly the local spur (sometimes called the Orion Spur; see below), which is a small piece of spiral arm in which the local Galactic magnetic field is confined. The blobs show the field coming towards the observer on one side and receding on the other. The structure seen is relatively local, i.e. within a kiloparsec or so of the observer.

I was very pleased to see this come out so clearly from an apparently unpromising data set, although we had to confine ourselves to large-scale features because of instabilities in the reconstruction of high-frequency components.