Past Events | Department of Astronomy and Astrophysics

2020

Winter 2020 Postdocs Symposium

3:00–5:00 pm ERC 401

Speakers: Dan Baxter, Cosmin Deaconu, Reed Essick, and Alex Alarcon Gonzalez
Organizers: Dan Baxter, Anne Gambrel, and Yiming Zhong

Mar 6

KICP colloquium: Tobias Marriage (Johns Hopkins University)

3:30–4:30 pm ERC 161

“The Cosmology Large Angular Scale Surveyor”

Mar 4

Chalk Talk: Gourav Khullar (UChicago) & Charles Mudd (UChicago)

12:00–1:00 pm ERC 501

Gourav Khullar (UChicago)
“Synthesizing Stellar Populations in Galaxies”

Charles Mudd (UChicago)
TBA

Mar 3

Open group seminar: Allison Strom (Carnegie Observatories)

3:30–4:30 pm ERC 419

“Rethinking metallicity: the quest to measure the chemistry of distant galaxies”

Feb 28

KICP seminar: Dhanesh Krishnarao (University of Wisconsin-Madison)

12:00–1:00 pm ERC 401

“The Inner Milky Way: Our New Closest LI(N)ER”

Feb 28

A&A Colloquium - Marco Velli (UCLA)

3:30–4:30 pm ERC 161

“Parker Solar Probe: Understanding Coronal heating and Solar Wind Acceleration”

The magnetic field is fundamental to solar activity and shapes the inter-planetary environment, as shown by the full three dimensional monitoring of the heliosphere provided by measurements from many past and present interplanetary and remote sensing spacecraft. Magnetic fields are also the source for coronal heating and the very existence of the solar wind; produced by the sun’s dynamo and emerging into the corona, magnetic fields become a conduit for waves, act to store energy, and then propel plasma into the Heliosphere in the form of Coronal Mass Ejections (CMEs). Magnetic fields are also at the heart of the generation and acceleration of Solar Energetic Particle (SEPs) that modify the space weather environment of the Earth and other planets.

Parker Solar Probe (PSP) was launched in August 2018 to carry out the first in situ exploration of the outer solar corona and inner Heliosphere. Direct measurements of the plasma in the closest atmosphere of our star should lead to a new understanding of the questions of coronal heating, solar wind acceleration, and the generation, acceleration and propagation of SEPs.

In this lecture I will start with an introduction to our present knowledge of the magnetized solar corona and wind before describing the PSP scientific objectives, orbit, and instrument suites, and showing results from the first three orbits. Emphasis will be on how PSP will confirm or falsify present wind models as well as the potential new discoveries stemming from the first exploration of the space inside the orbit of Mercury. I will also discuss how synergies with Solar Orbiter might lead us to accurately understand the state of the solar wind all the way from the corona into interplanetary space, a stepping stone for understanding the dynamics of active magnetized plasmas throughout the universe.

Feb 26

Special A&A Colloquium: Azadeh Maleknejad (Max Planck Institute for Astrophysics)

12:00–1:00 pm ERC 576

A new paradigm for particle cosmology

Modern cosmology has been remarkably successful in describing the Universe from a second after the Big Bang until today. However, our current understanding of the cosmos before that time is less precise. Moreover, cosmology profoundly involves particle theory beyond the Standard Model to explain its long-standing puzzles: the origin of the observed matter asymmetry, particle nature of dark matter, and cosmic inflation. In this colloquium, I will explain that relic axion-gauge fields in fractions of a second after the Big Bang can relate and explain these seemingly unrelated puzzles in early and late cosmology. As a smoking gun, such relics would provide a new window into the early Universe through primordial gravitational waves. Therefore, they are testable by future CMB missions.

Feb 25