Showing posts with label Lectures. Show all posts
Showing posts with label Lectures. Show all posts

Sunday, January 18, 2026

Listening to the early Universe - Studium General Marc Klein Wolt

Selfie with Dr. Marc Klein Wolt

I attended the lecture by Dr. Marc Klein Wolt which spoke of his mission to the back side of the Moon and his ideas about installing huge antenna's on the back side of the Moon.

Dr. Marc Klein Wolt, astrophysicist at Radboud University Nijmegen and director of the Radboud Radio Lab, is exploring the origin of the Universe by studying the redshifted 21-centimeter hydrogen line. This signal, emitted by neutral hydrogen, allows scientists to probe the so-called Cosmic Dark Ages, the era after the Big Bang and before the first stars and galaxies ignited.

As the Universe expanded, the original 21-cm signal was stretched, or redshifted, to much longer radio wavelengths (100m and more). Detecting this extremely faint radiation from Earth is nearly impossible due to radio interference and the blocking effects of Earth’s ionosphere. Therefor the idea to install equipment at the back side of the Moon.

In 2019, a radio antenna developed by Klein Wolt’s team flew with the Chinese Chang’e-4 mission, using the Queqiao relay satellite positioned behind the Moon. This location, permanently shielded from Earth’s radio noise, offers one of the quietest environments in the Solar System for radio astronomy.

By observing from lunar orbit, Klein Wolt aims to trace how the first cosmic structures formed from primordial hydrogen. His long-term vision includes building radio antennas on the lunar surface itself. These plans align with future European Space Agency (ESA) lunar initiatives, in which Europe seeks a scientific presence on and around the Moon.

The scientific importance of the 21-cm line is underscored by its inclusion on the Voyager Golden Record, sent into interstellar space as a universal cosmic reference. Together, lunar radio astronomy and international missions may soon reveal how darkness in the early Universe gave way to the first light.





The cosmic microwave background (CMB) was released about 380,000 years after the Big Bang during recombination, when electrons and protons combined to form neutral hydrogen. This was the first light that could travel freely through the universe. After that came the cosmic dark ages (roughly 380,000 to 100 million years), when the universe was mostly neutral hydrogen and no stars had formed yet. During this period, the 21 cm line from neutral hydrogen can be used to trace the distribution of matter. Later, the first stars and galaxies formed (~100–400 million years), emitting ultraviolet light that ionized hydrogen, beginning the reionization process, which was largely complete by about 1 billion years, weakening the 21 cm signal in ionized regions.

Sunday, January 4, 2026

ROS 2026 - Registration is open

The next Solar Observers’ Meeting (ROS) is scheduled for June 13–14, 2026, in Serbannes. Once again, the program will feature many instruments dedicated to solar observation in white light, calcium lines, and the H-alpha line for observing prominences, as well as the latest filter innovations. The Sol’Ex spectrograph will also be part of the event.

Registration is now open.



Friday, December 12, 2025

Conny Aerts - Asteroseismology

Conny's research covers stellar astrophysics, including stellar structure & evolution and variable stars. She is a pioneer of asteroseismology, which received a major boost thanks to the CoRoT (2006+), Kepler (2009+), and TESS (2018+) space missions. Prior to high-precision space photometry, Conny developed rigorous mathematical methods to detect and identify non-radial stellar oscillations in high-resolution time-series spectroscopy. Her team also designed and applied statistical classification methods in a machine-learning context, discoving numerous gravity-mode pulsators in space photometry. As Chair in Asteroseismology at the Radboud University Nijmegen, Conny introduced herself into the topic of subdwarf stars, their binarity and pulsations, with current focus on development and exploitation of BlackGEM in tandem with gravitational wave studies.

Conny gave a lecture  on thursday evening (11/12/2025) as part of an  Invited theatre lecture performance for Science Cafe De Kempen: “Asteroseismologie: ´ daar zit muziek in!” (in Dutch), Organised in Tabloo, Dessel, Belgium. 



Saturday, October 18, 2025

Lecture by Dr. Marcel van Daalen

 


During the annual JVS/VVS weekend (October 4th), Dr. Marcel van Daalen of the university of Leiden gave a lecture on the current status of our understanding of the universum. He talked about historical facts, observations and aswell inconsistencies. 




Saturday, July 12, 2025

JASON2025 @ Baron (France)- Report Out

Pascal Hilkens and Walter Swinnen

It’s June 21st and the official start of summer—and you can feel it, as it promises to be sunny and hot. On Friday evening, I had already packed the car with my suitcase of clothes, mounting equipment, telescope, and Sol’Ex. Johan L also stopped by briefly to deliver the new Sol’Ex (a new design by James R) that he had printed during the week. The device is 3D-printed in matte black material and looks very professional because of it.

After a short night’s sleep, I set off at 5:15 a.m. towards Diest to pick up Walter. And so we left at 5:30 a.m. heading to Baron (in the Oise department of the Hauts-de-France region), about 45 km northeast of Paris. It’s a 340 km drive, and we took the route through Brussels toward Mons and Valenciennes. After two hours of driving, we stopped near Cambrai for a pastry and a cup of coffee. After some issues, I finally managed to charge my electric car. Satisfied, we continued on our way and approached the first toll station. The toll is always a tense moment—will the Bip&Go work or not? And yes, everything worked fine.

I thought I had set the GPS to the exact location, but when it led us into the forest, we double-checked everything. After entering "Baron center," we were back on the right track.


In the village, a few signposts guide us to the location. We arrive right on time, and in the meadow next to the soccer field, there's already a pleasant buzz of activity. We register and are treated to a cup of coffee. From this point on, it's all French being spoken, which definitely takes some getting used to. We introduce ourselves and walk past the many set-up (solar) telescopes.




The program is changed, and Olivier Aguerre begins with his lecture on observing magnetic fields and the E-Corona using the Sol’Ex. He shares his experiences with us, and we get the chance to ask quite a few questions. Then it's time for lunch, and we sit at the table with Christian Buil and Valérie Desnoux. During our conversation, it becomes clear that the Sol’Ex collimator can be refocused when changing the wavelength. I had tested this before the meeting with very good results and was glad that Christian could confirm it. He admitted that he doesn’t talk much about this, as the Sol’Ex is a device that involves quite a few compromises.

One thing led to another, and I was able to hand over the new Sol’Ex by James R to Buil. He was very impressed by the print quality and the design. The device quickly made the rounds. Buil didn’t waste any time and took a lot of photos.







The next speaker is Dr. Allan Sacha Brun, an astrophysicist working at CEA (Commissariat for Atomic Energy and Alternative Energies), who takes us on a journey through the fascinating world of solar phenomena.



After the lecture, I set up my Sol’Ex setup and manage to take some recordings and compare them with others.



We continue exploring the various setups, many of which feature very impressive equipment.











Several participants have double and even triple-stacked H-alpha telescopes. All of them have placed a circular polarizer between the H-alpha filters. In the meadow, there are also some participants using the same AZ/EQ6 mount, and they confirm that scanning is only possible in one direction. In the other direction, it is not possible to perform vibration-free scanning. There are also a few harmonic mounts present, with the note that the scan speed may vary during acquisition. This is a kind of built-in safeguard that must be taken into account.

I take some time to talk with Florence Cornu, who is the program leader of Sol’Ex Pro-Am SOLAP, of which I am a member. She informs me that submitted images will be judged more strictly in terms of tilt deviation. Therefore, polar alignment and the Sol’Ex setup will need to be nearly perfect.

I check with Christian Viladrich on the status of the new edition of his book Solar Astronomy. According to the latest updates, he expects it to be ready in the first quarter of 2026.



It is now 7:00 PM, and the organizers (MARS60 – Mouvement Astronomique de la Région de Senlis) treat us to a snack and a drink. A little later, we sit down for dinner. This time, we’re at a table with Nic Spencer (Citizen Solar Astronomer, York, UK), Michael O’Connell (former Chairman of the Irish Federation of Astronomical Societies, Kildare, Ireland), and Filip Szczerek (better known as GreatAttractor and developer of IMPPG), with many interesting conversations.






After dinner, we drive to Senlis where we will spend the night at Hotel Grill Camp. It’s a fairly basic hotel, but it's only for one night. I’m also able to charge my car there. We sleep well, as it had been a long and tiring day—especially with temperatures reaching around 37°C.



In the morning, we enjoy a hearty breakfast and, after checking out, we drive back to Baron.

The weather is somewhat changeable, with occasional threatening clouds, but it remains dry. We meet up with Olivier to go over the practical side of capturing a magnetogram of the Sun. I have all the necessary equipment with me, which allows us to sort everything out fairly well.



I also speak with Valérie Desnoux about her software Inti and some issues I’ve encountered. She mentions that she is currently working on a newer version, and we manage to solve a few problems together. Afterward, Valérie and Christian Buil give a presentation on SunScan—the smaller sibling of the Sol’Ex, mainly intended for public outreach. The SunScan uses the same diffraction grating as the Sol’Ex and also features a built-in camera and Raspberry Pi. The images are transmitted via Wi-Fi to one or more smartphones. This last feature could be particularly useful for public demonstrations. I forward the information to Johan L, who expresses interest.



During lunch, we sit with Nicolas Godingen, a Frenchman currently working and living in Belgium. He focuses primarily on solar photography using mirror telescopes, whose mirrors have a special coating. These coatings are designed to primarily transmit H-alpha and Ca II wavelengths. He speaks very highly of the coating company MCM (https://www.mcm-optique.com/fr/). To reduce costs, several mirrors can be treated simultaneously in a vacuum chamber. I glance over at Walter—perhaps this is something for the future?

We attend another lecture by Christian Viladrich and Thierry Legault, who go each year to Saint-Véran for a week of solar photography. The location is at an altitude of 2000 meters, offering sunshine almost every day and excellent seeing conditions. They use telescopes with mirrors coated specifically to transmit only H-alpha and Ca II, as well as triple-stacked H-alpha telescopes. Their images and videos are absolutely stunning.

We take one last walk around the field, say our goodbyes to the participants, and if all goes well, we’ll see each other again at ROS 2026 (Rencontres des Observateurs Solaires) in Serbannes on June 13 and 14, 2026.

We head home, and with smooth traffic, we arrive around 7 PM—tired but satisfied.







Tuesday, June 17, 2025

JASON2025 June 21 & 22, 2025

Next weekend, June 21 and 22, MARS60 is organizing their Journées de l'Astronomie Solaire de l'Oise et du Nord @ Baron (France). My objective is to meet other Sol'Ex users and what's the next level.



Saturday, March 22, 2025

Space Weather Training STCE

This week I could attend the Space Weather training at STCE (Solar-Terrestrial Center of Excellence @Uccle Belgium). This introductionary training was open for all amateurs of the astronomy club VVS. In total 11 people participated the course.

The three main trainers (Petra, Elke and Jan) gave very well, detailed and interactive information about all aspects of space weather. Beside classroom lectures we participated a space weather forecast, visited the Uccle Solar Eqautorial Table (USET), Library of the Royal Observatorum and the headquarters of Solar radio-astronomy for Humain. 

A lot of information was given and how to understand the different parameters and how they are measured. I'm looking back to a succesfull two day training. Thx to STCE and all trainers. 


Attending Space Weather forecast meeting

Selfie with Walter in the Library

Library of Royal Observatorium

USET 

USET Control Room

Historical drawing with huge sunspot

The Solar Dome

Exercise 

left to right Ivo, Roel, Stijn,Pascal, Fleur, Niels, Claude, Jan, Petra, Walter, Elke, Rudy, Ann, Ruben





Sol'Ex Lecture @ Astronomy club Altair

My Sol'Ex project and Journey since 2023 was subject of my lecture @ Astronomy Club Altair in Sint-Truiden. About 14 people attended the lecture which took about 1h. Many questions were asked and could be answered.

After the lecture we could talk futher at the bar and a thank you gift was handed over by chairman of Altair, Steven Lambrechts. Looking back on a succesfull evening!



Click on image to see the lecture





Selfie with colleagues Jean-Marie and Walter

Chairman of Altair Steven Lambrechts 

Saturday, February 15, 2025

Studium Generalé with Prof dr Auke-Pieter Colijn and the XenonXT Project


Since 2017 I have been visiting Maastricht University on a regular basis as part of Studium Generalé. Studium Generalé provides excellent lectures as well as series of lectures that are always given by top professors or professionals.

Last Thursday, March 13, the missing universe was on the agenda by Prof. Dr. Auke-Pieter Colijn. He is a physicist who works as a professor of experimental astrophysics at the univ of Amsterdam and Utrecht. Around 6:30 pm I left for Maastricht and took Helios colleagues Walter and Fernando with me. For Walter it is already the most normal thing in the world, but for Fernando it was his first visit to Studium Generale. This time the lecture took place in the School of Business and Economics and not in the prestigious Minderbroedersberg. We were well on time and easily found a place in the grand auditorium. 



The lecture started with an overview of the size of the universe and how empty it actually is. All the matter we can observe makes up only 4% of our universe. The remaining 96% consists of something we don't know and therefore call dark energy and dark matter.


In Gran Sasso, Italy, at 1500m underground, is the Laboratori Nazionali del Gran Sasso (LNGS). Here deep underground they are looking for WIMPs or weakly interacting massive particles. These particles are possible candidates for dark matter. For the sake of completeness, all other candidates were also discussed.


To find the WIMP particles, a tank was built with 8000 kg of liquid Xenon, the so-called XenonNT project see https://xenonexperiment.org/ When a WIMP particle interacts with xenon, electrons and a photon will be released immediately. The electrons are led by an electric field to the top of the tank where they come into contact with gaseous Xenon and release another photon. The sequential release of two photons over a certain time interval is the characteristic of a WIMP. Despite the fact that the experiment has been working for several years, no dark matter was found.







Friday, December 27, 2024

Chart of Nuclides

I used to have a chart of Nuclides but can't find it any more :(
On line some interesting links to nuclides websites:


To buy a chart of nuclides, choose the one from Karlsruhe Nuclide Chart via https://nuklid.shop/

At the Tabloo Expoo a Nuclide chart was build in "glass" cubes with additional LED lights.  The X-Y axes are number of Protons and Neutrons, the vertical axe is Energy. The lower, the cubes, the more stable the isotope is. The lowest of all is iron - Fe.





Visiting Tabloo Dessel

Together with Helios Astronomy Club I visited Tabloo Expoo in Dessel (B). Tabloo is the brand-new visitor and meeting centre in Dessel about radioactivity, the management of radioactive waste and research into nuclear applications.