Given the recent surge in solar and geomagnetic activity, spectacular auroral displays have been visible down to the mid-latitudes several times since the beginning of 2024. But it is not always so easy to know when to go out, where to look, and how to take good pictures of the aurora. And what if the observations collected by seasoned and first-time aurora chasers could help in advancing the scie ...[Read More]
ST-ECS Networking Campfire – How to convene a scientific session
Convening a session at academic conferences is no doubt time-consuming, but they are also the primary catalysts for establishing a research network and significantly boosting your academic profile. Particularly for Early Career Scientists (ECS), the idea of convening a session can be fearful and many worry that they don’t know how to do it or whether they can wrap up the session smoothly. The ECS ...[Read More]
Meet our divisions ECS team that organized events throughout 2023-2024
Hi, this is your ST-ECS team 2023-2024. We are a group of Early Career Scientists (ECSs) of the Solar-Terrestrial (ST) division, and we organize events and activities with and for ST-ECS, both during the EGU General Assembly and throughout the year. Our aim is to increase the visibility of ECSs and provide you with opportunities for networking. Dr. Liliana Macotela, ECS Representative Lilia ...[Read More]
Events organized for early career scientists (ECS) by the ST-ECS Team during EGU24
The EGU General Assembly is around the corner, and we would like to advertise the events the Early-Career Scientist (ECS) Team of our Division have been preparing to create networking opportunities for ECSs. Solar-Terrestrial ECS Drinks: preGA Icebreaker Get-together for all ST ECSs before the opening reception. We’re meeting up at 15:00 hours in front of the entrance of the name badges coll ...[Read More]
Assessing the impact of chlorine ions on solar proton event induced ozone loss
Particle Precipitation High energy particles (e.g. electrons and protons) that precipitate at high latitudes can alter the chemical composition of the atmosphere by different photochemical reactions. This mainly happens due to primary collision processes and subsequent ion and neutral-chemistry reactions. Such reactions ordered by increasing energy are, for example, excitation, photo-dissoc ...[Read More]
ST-ECS Networking Campfire on “Time management strategies for research productivity”
Life in academia can be complex, involving handling multiple roles while developing and sustaining a successful career. Therefore, it can be challenging to balance research responsibilities with other commitments. Understandably, effective time management is essential for researchers to be productive and to achieve their goals, without sacrificing other important matters in life. The Early Career ...[Read More]
Exploring Magnetosheath Jets and their dependence on Solar Wind structures
Dayside of the Earth’s magnetic field Our understanding of the relationship between Earth’s magnetic field and the particles from the Sun that constantly bombard it, known as the solar wind, has significantly advanced in recent decades. The availability of numerous spacecraft measurements has provided valuable insights into this interaction. The solar wind, composed of high-speed particles c ...[Read More]
Why faculae “vanish” on active Suns
The Earth’s primary energy source is the radiative energy flux (i.e., the Total Solar Irradiance, TSI) from the Sun. Understanding the TSI or the solar irradiance output in particular wavelengths is important, as it is crucial for sustaining life of metabolisms on Earth and in answering the question of how life emerged on Earth. It has been shown that magnetic activity on the solar surface is one ...[Read More]
Events organised by the ST-ECS Team during EGU23
The General Assembly is around the corner, and we would like to advertise the events the early-career scientist (ECS) Team of our Division have been preparing to create networking opportunities for ECSs. Joint picnic for ST/PS/AS/EMRP ECSs (in-person only) When? Monday 24 April, 12:30–13:45 CEST Where? Meeting near the main entrance of the Austrian Center Vienna (ACV), before heading out to the Do ...[Read More]
Employing J burst observations made by LOFAR to determine the properties of large coronal loops
Large coronal loops around one solar radius in altitude are an important connection between the solar wind and the low solar corona. However, their plasma properties are not well studied, as standard X-ray and UV techniques are not suited to these low-density environments. How does temperature, pressure, and magnetic field strength evolve along these loops? Observable structures in radio emission ...[Read More]