Coronal hole picoflare jets are progenitors of both fast and Alfvénic slow solar wind
L. P. Chitta, Y. -M. Wang, R. Aznar Cuadrado(Max Planck Institute for Solar System Research), D. Calchetti, D. M. Hassler(Southwest Research Institute), C. Verbeeck, U. Schühle(Max Planck Institute for Solar System Research), Emil Kraaikamp, C. J. Owen(University College London), S. K. Solanki(Kyung Hee University), R. D'Amicis, T. S. Horbury(Imperial College London), A. N. Zhukov(Lomonosov Moscow State University), L. Teriaca(Max Planck Institute for Solar System Research), J. Hirzberger(Max Planck Institute for Solar System Research), L. Harra, S. Livi, A. Giunta(Oxfam), Z. Huang(Max Planck Institute for Solar System Research), D. Berghmans(Royal Observatory of Belgium), H. Peter, P. Louarn
Cited by 0
Related Papers
Emergence of genomic diversity and recurrent mutations in SARS-CoV-2
|Infection Genetics and Evolution|2020|897
The Solar Orbiter magnetometer
|Astronomy and Astrophysics|2020|292
The Solar Orbiter SPICE instrument
|Astronomy and Astrophysics|2019|145
Dynamics of thin current sheets associated with magnetotail reconnection
|Journal of Geophysical Research Atmospheres|2006|127
Solar and Heliospheric Phenomena in October–November 2003: Causes and Effects
|Cosmic Research|2004|127