Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Jozsef Kóta"'
Autor:
Vladimir Florinski, Juan Alonso Guzman, Jens Kleimann, Igor Baliukin, Keyvan Ghanbari, Drew Turner, Bertalan Zieger, Jozsef Kóta, Merav Opher, Vladislav Izmodenov, Dmitry Alexashov, Joe Giacalone, John Richardson
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 2, p 244 (2024)
This paper examines the geometry of interstellar magnetic field lines close to the boundary of the heliosphere in the direction of the unperturbed local interstellar magnetic field, where the field lines are spread apart by the heliopause (HP). Such
Externí odkaz:
https://doaj.org/article/15bdaeba106b48bcb91b5c8b8e4ae59c
Autor:
Merav Opher, John Richardson, Gary Zank, Vladimir Florinski, Joe Giacalone, Justyna M. Sokół, Gabor Toth, Sanlyn Buxner, Marc Kornbleuth, Matina Gkioulidou, Romina Nikoukar, Bart Van der Holst, Drew Turner, Nicholas Gross, James Drake, Marc Swisdak, Kostas Dialynas, Maher Dayeh, Yuxi Chen, Bertalan Zieger, Erick Powell, Chika Onubogu, Xiaohan Ma, Ethan Bair, Heather Elliott, Andre Galli, Lingling Zhao, Laxman Adhikari, Masaru Nakanotani, Matthew E. Hill, Parisa Mostafavi, Senbei Du, Fan Guo, Daniel Reisenfeld, Stephen Fuselier, Vladislav Izmodenov, Igor Baliukin, Alan Cummings, Jesse Miller, Bingbing Wang, Keyvan Ghanbari, Jozsef Kota, Abraham Loeb, Juditra Burgess, Sarah Chobot Hokanson, Cherilyn Morrow, Adam Hong, Andrea Boldon
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
Most stars generate winds and move through the interstellar medium that surrounds them. This movement creates a cocoon formed by the deflection of these winds that envelops and protects the stars. We call these “cocoons” astrospheres. The Sun has
Externí odkaz:
https://doaj.org/article/886a0a29d9a74a468265e495a7e588ed
Publikováno v:
The Astrophysical Journal, Vol 973, Iss 2, p 118 (2024)
The interpretation of gamma-ray emission originating from the solar disk (0.5° in angular size) as due to the interaction of Galactic Cosmic Rays (GCRs) with the solar atmosphere has remained a central challenge in solar physics. After the seminal w
Externí odkaz:
https://doaj.org/article/6fef6caa896e4751810fe66e2a94932a