Temperature and differential emission measure evolution of a limb flare on 13 January 2015

Autor: Bröse, Malte, Warmuth, Alexander, Sakao, Taro, Su, Yang

Publikováno v: Volume 663, A18, July 2022

Spatially unresolved observations show that the cooling phase in solar flares can be much longer than theoretical models predict. It has not yet been determined whether this is also the case for different subregions within the flare structure. We aim

Externí odkaz: http://arxiv.org/abs/2406.13339

A Space Weather mission concept: Observatories of the Solar Corona and Active Regions (OSCAR)

Autor: Strugarek Antoine, Janitzek Nils, Lee Arrow, Löschl Philipp, Seifert Bernhard, Hoilijoki Sanni, Kraaikamp Emil, Mrigakshi Alankrita Isha, Philippe Thomas, Spina Sheila, Bröse Malte, Massahi Sonny, O’Halloran Liam, Blanco Victor Pereira, Stausland Christoffer, Escoubet Philippe, Kargl Günter

Publikováno v: Journal of Space Weather and Space Climate, Vol 5, p A4 (2015)

Coronal Mass Ejections (CMEs) and Corotating Interaction Regions (CIRs) are major sources of magnetic storms on Earth and are therefore considered to be the most dangerous space weather events. The Observatories of Solar Corona and Active Regions (OS

Externí odkaz: https://doaj.org/article/898d7fa323444942a0d1c7a3478b8063

A Space Weather Mission Concept: Observatories of the Solar Corona and Active Regions (OSCAR)

Autor: Strugarek, Antoine, Janitzek, Nils, Lee, Arrow, Löschl, Philipp, Seifert, Bernhard, Hoilijoki, Sanni, Kraaikamp, Emil, Mrigakshi, Alankrita Isha, Philippe, Thomas, Spina, Sheila, Bröse, Malte, Massahi, Sonny, O'Halloran, Liam, Blanco, Victor Pereira, Stausland, Christoffer, Escoubet, Philippe, Kargl, Günter

Coronal Mass Ejections (CMEs) and Corotating Interaction Regions (CIRs) are major sources of magnetic storms on Earth and are therefore considered to be the most dangerous space weather events. The Observatories of Solar Corona and Active Regions (OS

Externí odkaz: http://arxiv.org/abs/1409.0458

Publisher Correction: Fine structures of a solar type III radio bursts observed with LOFAR.

Autor: Dabrowski, Bartosz¹ (AUTHOR) bartosz.dabrowski@uwm.edu.pl, Wolowska, Aleksandra (AUTHOR), Vocks, Christian (AUTHOR), Magdalenić, Jasmina^2,3 (AUTHOR), Zhang, Peijin^4,5 (AUTHOR), Flisek, Pawel (AUTHOR), Bröse, Malte^6,7 (AUTHOR), Morosan, Diana E. (AUTHOR), Krankowski, Andrzej (AUTHOR), Fron, Adam (AUTHOR), Mann, Gottfried (AUTHOR), Zucca, Pietro (AUTHOR), Bisi, Mario (AUTHOR), Fallows, Richard (AUTHOR), Gallagher, Peter (AUTHOR), Marqué, Christophe (AUTHOR), Matyjasiak, Barbara (AUTHOR), Rothkaehl, Hanna (AUTHOR)

Publikováno v: Acta Geophysica. Oct2024, p1-2.