We are the Solar Physics/MHD group based in the Mathematics Department at Durham University, tweeting about all things solar and/or magnetohydrodynamic!
When does the magnetic helicity change, but you get no reconnection? (come back this is not a solar nerd joke!) Turns out pretty much all the time! See here for details
https://t.co/mXb7sjoFhV
Some (late) research advent highlights! @Pecnut 's simulations of elastic tubes (sperm's!) gihting their way through a springy network (mucus), horrific numerics done with style! (https://t.co/oRkGXObpx1)
📢New paper alert, how to recognise regions of reconnective activity in turbulently reconnective plasma's with the folk at UCLA and their big plasma tube:
https://t.co/3XTtaGjXRd
Though near-blind and dwelling underground, the eyes of the African Ansell's mole-rat can sense magnetic fields, according to new research in @RSocPublishing#Interface. See the full article: https://t.co/P3529dPNrh
What we have been up to this year 4: Adam Townsend has had accepted a frankly intimidating treatise on the modelling of active filaments in fluids:
https://t.co/Mt5XGJAtZQ
What we have been up to this year 3: Peter Wyper has been CO-I on project Hazel Wyper, a very demanding effort with PI Sarah, he has also done great things on sympatheic (ish) eruptions which will appear soon....
What we have been up to this year 2: Chris Prior has been looking into wavelet decompositions of magnetic helicity, a better means of characterising inhomogeneity than standard Fourier methods: https://t.co/jpmfwJlr4N
What we have bee up to this year 1: Anthony Yeates asks how careful we should be about representing the structure of new active regions in SFT models, in short very, but he has made python code to do it properly for you!
#EditorsChoice:
Anthony R. Yeates, "How Good Is the Bipolar Approximation of Active Regions for Surface Flux Transport?". #SolarPhysics 295, 119 (2020). https://t.co/hv5DZAioMJ #BMR#HMI#SDO#SHARP