Author: sharp_adm

The fifth SHARP Progress meeting took place on 3rd December, 2021.

The 63rd Annual Meeting of the APS Division of Plasma Physics was held from Monday to Friday, November 8–12, 2021 in Pittsburgh, PA. During the meeting two sessions of the Mini-Conference on Collisionless Shocks in Laboratory and Space Plasmas were organized (co-conveners: N. Pogorelov, M. Gedalin (SHARP), D. Schaeffer). Most of the topics of the mini-confererence were directly relevant to the research within SHARP.

The talk CM10.00007: Modeling Solar Wind Interaction with the Local Interstellar Medium using Kinetically-Derived Rankine-Hugoniot Conditions for Pickup Ions (N. Pogorelov, M. Gedalin (SHARP), V. S. Roytershteyn, R. K. Bera, F. Fraternale, W. P. Smith, M. Zhang) includes the results obtained by M. Gedalin within the work on Workpackage 2 and 3.
The talk CM10.00006: Kinetic Simulations of the Behavior of Pickup Ions in the Vicinity of a Collisionless Shock (V. S. Roytershteyn, P. F. Kilian, M. Gedalin (SHARP), N. Pogorelov) is also related to the research within the SHARP project.

The first SHARP Science meeting took place on 16th November, 2021.

In September, Dmitry Prokhorov started to work on X-ray polarimetry in the group led by Jacco Vink at the University of Amsterdam (UvA). Dmitry will analyze data from the Imaging X-ray Polarimetry Explorer for performing a polarimetric study of supernova remnants to characterize particle acceleration at their shock fronts.

As of October, Emanuele Greco joined UvA as a member of the SHARP team. He will deal with non-thermal emission due to synchrotron radiation in supernova remnants by analyzing observations collected in the X-ray energy band. In particular, he will look for spectral signatures of jittering radiation in young remnants such as Cassiopeia A, Tycho and SN 1006.

The Mach number is one of the most important parameters of collisionless shocks. The accuracy of its observational determination is compromised by several complications. Incomplete measurements of plasma parameters significantly contribute to the uncertainty, along with the errors of the normal determination. A set of CLUSTER observed shocks is analyzed using several methods for finding the shock normal and to circumvent the shortcomings of the plasma data. A relation between the maximum magnetic compression and the Alfvénic Mach number is established. It is proposed as a proxy for the Mach number estimate when measurements are incomplete.

Full article:
Gedalin, M., Russell, C. T., Dimmock, A. P. (2021). Shock Mach number estimates using incomplete measurements. Journal of Geophysical Research: Space Physics, 126, doi: 10.1029/2021JA029519

License: CC BY-NC-ND 4.0

The fourth SHARP Progress meeting took place on 3rd September, 2021.

In August, Andreas Johlander joined IRF as a member of the SHARP team. He will work on improving our understanding of how particles behave during shock rippling and nonstationarity. In addition, he will investigate the characteristics of waves and instabilities as well as their roles in regulating the macroscopic properties of the shock front.

Andrew Dimmock gave a presentation entitled “An MMS bow shock database using machine learning: EU H2020 SHARP project” at the summer GEM virtual workshop (https://gemworkshop.org/) in the focus group “Particle Heating and Thermalization in Collisionless Shocks in the MMS Era”. The presentation provided details of the identification of terrestrial bow shocks using machine learning classification of the ion phase space distribution functions and the SHARP project. An overview of the SHARP terrestrial database was presented, as well as quick look plots, and the online functionality available to the wider community.

Click here to view the presentation or visit the Publications and Presentations page.