Upflows in solar active regions - producing a mix of abundances that can feed into the solar wind
Upflows in solar active regions - producing a mix of abundances that can feed into the solar wind
Louise Harra1, Krzysztof Barczynski2, Cristina H Mandrini3, David Brooks4, German Cristiani5, Alphonse C Sterling6, Udo Schühle7, Valentin Martinez-Pillet8, David Berghmans9, F Auchere10, Regina Aznar Cuadrado7, Eric Buchlin10, Lakshmi Pradeep Chitta11, Emil Kraaikamp9, David Long12, Sudip Mandel11, Susanna Parenti13, Hardi Peter7, Luciano Rodriguez14, Philip Smith15, Luca Teriaca7, Cis Verbeeck9 and Andrei Zhukov16, (1)PMOD WRC Physical Meteorological Observatory Davos and World Radiation Center, Davos Dorf, Switzerland, (2)ETH-Zurich and PMOD/WRC, Davos, Switzerland, (3)Instituto de Astronomía y Física del Espacio, Buenos Aires, Argentina, (4)George Mason University, Sagamihara, Japan, (5)Institute of Space Astronomy and Physics Buenos Aires, Buenos Aires, Argentina, (6)NASA Marshall Space Flight Center, Huntsville, AL, United States, (7)Max Planck Institute for Solar System Research, Göttingen, Germany, (8)National Solar Observatory, Boulder, CO, United States, (9)Royal Observatory of Belgium, Brussels, Belgium, (10)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France, (11)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (12)University College London, London, United Kingdom, (13)Institut d'Astrophysique de Paris, Paris, France, (14)SIDC, Royal Observatory of Belgium, Uccle, Belgium, (15)UCL - Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, United Kingdom, (16)Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia