EGU Guest blogger

New auroral dunes discovered through citizen science

Maxime Grandin and Minna Palmroth April 14, 2020

Two simultaneous pictures of the dunes on 7 October 2018 from (a) Laitila (by Pirjo Koski) and (b) Ruovesi (by Rami Valonen), where six fingertips were identified to determine their altitude. © Palmroth et al. (2020) / CC BY 4.0

The region of the Earth’s atmosphere lying at altitudes between about 80 and 120 km, corresponding to the mesosphere–lower thermosphere–ionosphere (MLTI), is often referred to as the “ignorosphere”, because its observation is so challenging that only a handful of measurements of its composition, temperature and other physical parameters have been obtained over the last few decades. It is, however, ...[Read More]

Chasing solar storms as an early career scientist

authored by Erika Palmerio, edited by Luke Barnard November 29, 2019

Hello! My name is Erika Palmerio and I am a newly qualified Dr in space physics from the University of Helsinki, Finland. In this blog post I will talk about my PhD research and my future career plans. The title of my PhD dissertation is “Magnetic structure and geoeffectiveness of coronal mass ejections”. Coronal mass ejections (or CMEs) are huge and spectacular clouds of magnetic field and plasma ...[Read More]

New insights to the north-south asymmetries of auroral features

Jone Peter Reistad February 14, 2019

Aurora Borealis above the EISCAT Svalbard Radar. Credit: Jone Peter Reistad

Recent research on the simultaneous displays of aurora in both hemispheres have lead to new knowledge of how large-scale asymmetries in the global magnetic field configuration can arise and be mitigated. This new understanding is contrary to what has been the consensus in the field, and was recently highlighted in a press release from the American Geophysical Union, followed by attention from nume ...[Read More]

Web-based Tools for Forecasting Solar Particle Events and Flares

Athanasios Papaioannou January 14, 2019

The effect of particles in the Bastille day event. Credit: http://sidc.be/news/233/welcome.html

The presence of Solar Energetic Particles (SEPs) poses a serious health risk to humans in space, can result in increased radiation doses for high-latitude aircraft flights and constitutes a serious hazard for the micro-electronics and other hardware elements of satellites, aircraft and launchers. These groups of end users need reliable forecasts of possible enhancements in the radiation flux level ...[Read More]

EGU for Early Career Scientists

Jone Peter Reistad November 16, 2018

Austria International Center, Vienna. Image credit: EGU/Stephanie McClellan

This months post is written by the ST Divisions Early Career Scientist representative, Theresa Rexer. Are you ready for the EGU general assembly 2019? Got your abstract ready and submitted? No, what? Too early you say? No funds? As your Early Career Scientist Representative, let me tell you why now is the perfect time to start planning your trip to Vienna in April next year. Especially if you are ...[Read More]

A close-up journey to the Sun: The Parker Solar Probe Mission

Athanasios Papaioannou October 24, 2018

Artist’s concept of the Parker Solar Probe spacecraft approaching the sun. Credit: NASA/Johns Hopkins APL/Steve Gribben

Almost two months ago, in August 12, 2018 Parker Solar Probe (PSP) launched by NASA on a Delta IV Heavy rocket from Cape Canaveral, Florida. This is a long-awaited mission from the Heliospheric community. The first to explore the Sun within distances of ~0.167 AU (or 25 million kilometers) at its perihelia. Its ancestors were the successful Helios -A and -B spacecraft, a pair of probes launched in ...[Read More]

Cosmogenic Radionuclides – The quest of studying the solar activity of thousands of years

Athanasios Papaioannou September 18, 2018

Figure 1: Sketch of the processes involved in order to model the atmospheric production of the cosmogenic radionuclides. Courtesy K. Herbst

Thanks to the invention of the Neutron Monitor in 1948 and multiple spacecraft which monitor the cosmic ray environment since 1970’s we now have a constant record of the solar activity over almost 70 years. Information prior to this space era, however, are rare and take us back in time only to the late 1930s, when ionization chambers have been introduced. This of course allows us only a narr ...[Read More]

The average magnetic field and polar current system (AMPS) model

Jone Peter Reistad June 15, 2018

Example of field aligned (red/blue) currents from both polar regions from the AMPS model. Grey pins represent the full horizontal current vector. The plot was made with the following input to the model: Solar Wind velocity: 350 km/s, IMF Bz: -8 nT, IMF By: -8 nT, dipole tilt angle: 20 degrees, F10.7: 80 sfu.

In this month’s post, Karl Magnus Laundal explains a newly developed empirical model for the full high latitude current system of the Earth’s ionosphere, AMPS (Average Magnetic field and Polar Current System). The model is available and documented in python code, published under the acronym pyAMPS. The community is invited to download and explore the electric currents and magentic fiel ...[Read More]

Prof. Ilya Usoskin – A discussion with an inquiry mind

Athanasios Papaioannou May 16, 2018

In Ancient Greece, the Sun was believed to be a god named Helios, who drove his shining carriage pulled by a quadriga along a dangerous and unpaved path through the sky. This was probably the first model of the Sun. Nowadays, we not only have a somewhat better theory but also know that, even during the Ancient Greek era, the Sun was not exactly like in this picture (from http://www.theoi.com/Titan/Helios.html)

In the May issue of the Life of a Scientist we have the pleasure to talk to Prof. Ilya Usoskin from the Univeristy of Oulu, Finland. Among numerous things, he is the head of the Oulu Cosmic Ray station and receipent of this year’s Julius Bartels EGU Medal; a decision that was based: “on his contributions to the understanding of the heliosphere, long-term changes in the solar activity ...[Read More]

Report from the 2018 EGU General Assembly

Jone Peter Reistad April 20, 2018

EGU venue. Credit: EGU/Stephanie McClellan

Last week the 2018 General Assembly were held in Vienna. Gathering 15 075 scientists from 106 countries, this is the most important EGU event throughout the year. Summarizing what happened during the week is an impossible task, as a meeting like this is way more than the 666 individual sessions convened and the 11 128 posters presented during the week. However, in this post I will point to some of ...[Read More]