Galactic cosmic rays

There’s a recent Nature Communications paper by Svensmark et al. called [i]ncreased ionization supports growth of aerosols into cloud condensation nuclei. The basic idea is that cosmic rays (energetic particles typically accelerated by shock waves) can influence the growth of aerosol particles that can then act as cloud nucleation sites. This may, therefore, play some kind of role in climate change.

The problem is that this idea has been around for quite some time and has essentially been pre-bunked. There’s a relevant Realclimate review called a cluttered story of little success. In fact, if you search Realclimate for Svensmark, you get a number of posts that cover this topic.

There have also been recent CERN results which suggest that the Sun-clouds connection takes a beating. The new paper has also not be all that well received.

It did, however, remind of something that I thought I would add here. I used to work with someone called Gary Zank, who was involved in research that was used to suggest that maybe dinosaurs were wiped out by genetic mutations from cosmic rays. The basic idea is that the Sun has a wind that blows a bubble of magnetised plasma – called the Heliosphere – into the interstellar medium. This acts to shield the inner Solar System from galactic cosmic rays.

However, the Solar System actually moves through the interstellar medium. The size of this bubble depends on the density and temperature of the local interstellar medium. Currently we’re in a warm, diffuse region, and so the bubble extends out to well beyond Pluto. However, when we are in a cold, dense region, it may only extend to about the orbit of Jupiter; much smaller than it is today. This would mean that the local cosmic ray flux would be much higher than when the bubble is larger. It is thought that we were in a denser region about 66 million years ago and, hence, maybe the enhance cosmic ray flux wiped out the dinosaurs.

I don’t think that is really regarded as a viable explanation. However, it does suggest that the local cosmic ray flux could vary quite substantially on these timescales. If cosmic rays can play a role in cloud formation, and hence our climate, you might expect to see some kind of signal in our past temperatures. I even found a paper that discusses exactly this, saying

We have demonstrated that the cosmic ray spectra at the Earth, particularly that of anomalous protons can vary by
orders of magnitude even for moderate changes in the interstellar medium……The assumed changes
in the state of the interstellar medium certainly occur along the galactic orbit of the Sun on time scales of a few thousand to a few million years. In conclusion, we state that, on these time scales, if the cosmic ray–climate link will be confirmed, one should consider an effect of interstellar–terrestrial relations on the climate on Earth.

As far as I’m aware, there is no indication of such a signal in our past climate. If, as suggested above, the cosmic ray flux vary by orders of magnitude, you might expect such a signal to be easy to find.

It seems highly unlikely that any cosmic ray effect on clouds (if there even is one) can be large enough to be climatically relevant. As far as I can tell, this recent paper is simply another attempt to suggest that our climate is somehow very sensitive to small changes in something that isn’t CO2 so as to imply that maybe it isn’t sensitive to much larger changes in CO2 itself.

Something I meant to include in the post, but forgot to do, was to point out something odd about Svensmark et als. reference list. This comes from a post by Ari Jokimaki. They do not cite a paper by Kulmala et al. called Atmospheric data over a solar cycle: no connection between galactic cosmic rays and new particle formation , but do cite earlier papers by the same author. As Ari points out, Svensmark et al. seems to ignore a number of recent papers that appear to contradict what they’re suggesting in this new paper.

This entry was posted in Climate change, Climate sensitivity, ClimateBall, Global warming, Science, Sound Science (tm) and tagged , , , , , , , . Bookmark the permalink.

11 Responses to Galactic cosmic rays

  1. Pat Cassen says:

    As far as I’m aware, there is no indication of such a signal in our past climate. If…the cosmic ray flux vary by orders of magnitude, you might expect such a signal to be easy to find.

    One might also expect to find a prominent signal in meteoritical cosmogenic nuclides. Apparently there is no evidence for such strong variations:
    The Galactic Cosmic Ray Intensity over the Past 106–109 Years as Recorded by Cosmogenic Nuclides in Meteorites and Terrestrial Samples

  2. Pat,
    Interesting, thanks. I wonder what that implies about the suggestion that we might expect some variation as the Solar System moves through the inter-galactic medium? I think the latter doesn’t particularly influence the very high energy cosmic rays.

  3. This was discussed at the AGU
    Solar-Driven Variation in the Atmosphere of Uranus

    The power spectra comparison appears stronger than directly comparing the time-series. Also works for Neptune.

  4. Harry Twinotter says:

    It doesn’t look like the earth’s magnetic field flipping every now and again has influenced climate, either. It stands to reason that the earth’s magnetic field disappearing would let more cosmic rays strike the atmosphere.

  5. dikranmarsupial says:

    It is hard to see how this made it through peer review when it cites early work on the CLOUD project, but not it’s negative (for the argument of the paper) outcome. Surely reviewers competent to review the paper would be aware that the CLOUD project doesn’t support Svensmark’s hypothesis?

  6. I expect Svensmark will be a shoe-in for the Red Team, which may need reinforcements given the timely leak of Heartland’s Christmas wish list .

  7. Andrew Dodds says:

    Harry – it’s a bit more complex than that – the field never disappears although the strength does reduce. But yes, there are, as far as I am aware, no noticeable effects of field reversals on climate or biosphere.

  8. Andrew,
    IIRC, what happens is that the dipole moment disappears and you end up with a quadrupole field, which would mean – I think – aurorae at the poles and at the equator. As you say, though, the field does not actually disappear.

  9. Eli Rabett says:

    Somewhere awaiting a science reporter is the story of the breakup btw. Svensmark and Kirby. It was….Eli might speculate. . . not pleasant

  10. Pingback: Some curious things about Svensmark et al. reference list

  11. D. Voorthuyzen says:

    about that signal in our past climate:
    It is, however, possible to obtain information about variations in cosmic rays in the years
    before neutron monitors became available. When energetic cosmic rays collide with the
    atoms of the atmosphere, new elements are produced. These elements are referred to as
    ‘cosmogenic isotopes’. Examples are beryllium-10, carbon-14 and chlorine-36. When the
    cosmic ray flux is high, the production of cosmogenic isotopes is also high, and vice versa
    when the flux is low. Variations in the quantity of cosmogenic isotopes therefore provide
    information on the variations in the cosmic-ray flux. For example, beryllium-10 (10Be) is produced high in the Earth’s atmosphere by cosmic rays. The 10Be atoms can then stick to small
    aerosols (molecular clusters floating in the air), and sometimes they become incorporated
    into snowflakes. If these fall somewhere where they will not melt, for example the Greenland
    icesheet, then by taking ice-cores and measuring the content of 10Be atoms in each dated
    layer of ice, a record of 10Be production, and thereby an indirect measure of past cosmic ray
    flux, is obtained.

Leave a Reply

Fill in your details below or click an icon to log in: Logo

You are commenting using your account. Log Out /  Change )

Twitter picture

You are commenting using your Twitter account. Log Out /  Change )

Facebook photo

You are commenting using your Facebook account. Log Out /  Change )

Connecting to %s

This site uses Akismet to reduce spam. Learn how your comment data is processed.