Slow solar wind sources - high-resolution observations with a stereoscopic view.
Slow solar wind sources - high-resolution observations with a stereoscopic view.
Krzysztof Barczynski1, Louise K Harra2, Conrad Schwanitz3,4, David Berghmans5, F Auchere6, Regina Aznar Cuadrado7, Eric Buchlin6, Lakshmi Pradeep Chitta8, Emil Kraaikamp5, David Long9, Sudip Mandel8, Susanna Parenti10, Hardi Peter7, Luciano Rodriguez11, Udo Schühle7, Philip Smith12, Luca Teriaca7, Cis Verbeeck5 and Andrei Zhukov13, (1)ETH-Zurich and PMOD/WRC, Davos, Switzerland, (2)Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, Davos Dorf, Switzerland, (3)PMOD/WRC, Davos, Switzerland, (4)ETH Zürich, Zürich, Switzerland, (5)Royal Observatory of Belgium, Brussels, Belgium, (6)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France, (7)Max Planck Institute for Solar System Research, Göttingen, Germany, (8)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (9)University College London, London, United Kingdom, (10)Institut d'Astrophysique de Paris, Paris, France, (11)Observatoire Royal de Belgique, Brussel, Belgium, (12)UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, United Kingdom, (13)Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia