Speaker
Dr
Ashley Bransgrove
(Princeton University, PCTS)
Description
Radio pulsars display a range of puzzling long-term variability in their magnetospheric emission and spin-down. In this talk I will discuss the mechanisms for internal magnetic field evolution of pulsars, how it differs from the MHD of classical conducting fluids, and how the neutron star interior couples to the magnetosphere and its radiation.
| Presenter's Name | Ashley Bransgrove |
|---|---|
| Presenter's Email Address | [email protected] |
| Keywords | Neutron stars, plasma physics, magnetospheres, radiation, superconductivity |
| Recording Permission | YES |
| Virtual Audience Permission | YES |
| Photography Permission | YES |
Primary author
Dr
Ashley Bransgrove
(Princeton University, PCTS)
External references
- 25030148
- d9e78ad3-c789-4375-9dfa-b9eef0e0cd8c
