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Catalyst for large-scale CO2 methanisation

https://www.mpg.de/21374612/co2-methane-methanisation-energy-storage?c=11970732

Core-shell catalysts developed by a team led by Kai Sundmacher at the Max Planck Institute for Dynamics of Complex Technical Systems lay the groundwork for the extensive conversion of carbon dioxide into methane. A key advantage lies in their ability to curtail the excess heat generated during CO2 methanization, mitigating potential damage to the catalyst.
Fluctuating electricity supply: Offshore wind parks sometimes supply more electricity

Catalyst for large-scale CO2 methanisation

https://www.mpg.de/21374612/co2-methane-methanisation-energy-storage?c=11863417

Core-shell catalysts developed by a team led by Kai Sundmacher at the Max Planck Institute for Dynamics of Complex Technical Systems lay the groundwork for the extensive conversion of carbon dioxide into methane. A key advantage lies in their ability to curtail the excess heat generated during CO2 methanization, mitigating potential damage to the catalyst.
Fluctuating electricity supply: Offshore wind parks sometimes supply more electricity

Sind Passatwindwolken als Einzelgänger oder in der Gruppe effektiver?

https://www.mpg.de/21278584/mpimet_jb_2023?force_lang=de

Passatwindwolken sind kleine Haufenwolken, die selten eine Höhe von mehr als 4 km erreichen aber weite Teile der tropischen Ozeane bedecken. Weil sie Sonnenstrahlen reflektieren und langwellige Wärmestrahlung effektiv in den Weltraum abgeben, spielen sie eine wichtige Rolle bei der Kühlung unserer Erde. Wie effektiv diese Wolken Niederschlag bilden und wie sich Niederschlagprozesse auf ihre Empfindlichkeit gegenüber Störungen auswirken – ob sich zum Beispiel ihre kühlende Wirkung mit der Klimaerwärmung abschwächt – können wir dank einer großangelegten Messkampagne nun besser verstehen.
Are trade wind clouds more effective solitary or in groups? 

Catalyst for large-scale CO2 methanisation

https://www.mpg.de/21374612/co2-methane-methanisation-energy-storage

Core-shell catalysts developed by a team led by Kai Sundmacher at the Max Planck Institute for Dynamics of Complex Technical Systems lay the groundwork for the extensive conversion of carbon dioxide into methane. A key advantage lies in their ability to curtail the excess heat generated during CO2 methanization, mitigating potential damage to the catalyst.
Fluctuating electricity supply: Offshore wind parks sometimes supply more electricity

Catalyst for large-scale CO2 methanisation

https://www.mpg.de/21374612/co2-methane-methanisation-energy-storage?c=12035149

Core-shell catalysts developed by a team led by Kai Sundmacher at the Max Planck Institute for Dynamics of Complex Technical Systems lay the groundwork for the extensive conversion of carbon dioxide into methane. A key advantage lies in their ability to curtail the excess heat generated during CO2 methanization, mitigating potential damage to the catalyst.
Fluctuating electricity supply: Offshore wind parks sometimes supply more electricity

Catalyst for large-scale CO2 methanisation

https://www.mpg.de/21374612/co2-methane-methanisation-energy-storage?c=154455

Core-shell catalysts developed by a team led by Kai Sundmacher at the Max Planck Institute for Dynamics of Complex Technical Systems lay the groundwork for the extensive conversion of carbon dioxide into methane. A key advantage lies in their ability to curtail the excess heat generated during CO2 methanization, mitigating potential damage to the catalyst.
Fluctuating electricity supply: Offshore wind parks sometimes supply more electricity

Gamma light from a nova

https://www.mpg.de/18414085/gamma-light-from-a-nova

or the first time, it has been possible to observe the eruption of a nova in very high-energy gamma light and to follow the illumination and subsequent fading over a period of one month. The researchers combined the data from the H.E.S.S. observatory with those from the Fermi satellite and gained insights into the processes underlying the emission of gamma rays. The scientists were surprised to find that the nova apparently accelerates particles to the theoretical limit.
Particles are accelerated at these shock fronts, which collide with the dense wind

Überraschungen bei höchsten Energien – Fortschritte in der Hochenergie-Astrophysik

https://www.mpg.de/4693963/Hochenergie_Astrophysik?c=1070738

Beobachtungen bei höchsten Energien haben wichtige fundamentale Aufschlüsse über die astrophysikalischen Prozesse in kosmischen Objekten ermöglicht. Sie haben uns dem Verständnis aktiver Galaxien wie M87 und unserer Milchstraße entscheidend näher gebracht.
In diesem Szenario treibt ein mehrere 100 km/s schneller Wind aus Protonen der Kosmischen