Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Jackie Villadsen"'
Autor:
J. Sebastian Pineda, Jackie Villadsen
Publikováno v:
Nature Astronomy. 7:569-578
Observing magnetic star-planet interactions (SPI) offers promise for determining magnetic fields of exoplanets. Models of sub-Alfv\'enic SPI predict that terrestrial planets in close-in orbits around M~dwarfs can induce detectable stellar radio emiss
Publikováno v:
Nature.
Autor:
R. O. Parke Loyd, James Paul Mason, Meng Jin, Evgenya L. Shkolnik, Kevin France, Allison Youngblood, Jackie Villadsen, Christian Schneider, Adam C. Schneider, Joe Llama, Tahina Ramiaramanantsoa, Tyler Richey-Yowell
Coronal mass ejections (CMEs) are a prominent contributor to solar system space weather and might have impacted the Sun's early angular momentum evolution. A signal diagnostic of CMEs on the Sun is coronal dimming: a drop in coronal emission, tied to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::651171bb07d714ecf47d986fe50a6315
http://arxiv.org/abs/2207.05115
http://arxiv.org/abs/2207.05115
Publikováno v:
Proceedings of the International Astronomical Union. 11:191-195
High-cadence spectroscopy of solar and stellar coherent radio bursts is a powerful diagnostic tool to study coronal conditions during magnetic reconnection in flares and to detect coronal mass ejections (CMEs). We present results from wide-bandwidth
Autor:
Gregg Hallinan, Jackie Villadsen
Publikováno v:
The Astrophysical Journal. 871:214
Coherent radio bursts detected from M dwarfs have some analogy with solar radio bursts, but reach orders of magnitude higher luminosities. These events trace particle acceleration, powered by magnetic reconnection, shock fronts (such as formed by cor
Publikováno v:
The Astrophysical Journal. 857:133
As part of a wider search for radio emission from nearby systems known or suspected to contain extrasolar planets, ε Eridani was observed by the Jansky Very Large Array (VLA) in the 2–4 GHz and 4–8 GHz frequency bands. In addition, as part of a
We present the first detections of thermal radio emission from the atmospheres of solar-type stars {\tau} Cet, {\eta} Cas A, and 40 Eri A. These stars all resemble the Sun in age and level of magnetic activity, as indicated by X-ray luminosity and ch
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7bef61b7d2823564e0ef71d28590747b
http://arxiv.org/abs/1405.2341
http://arxiv.org/abs/1405.2341
Autor:
Jackie Villadsen, Gregg Hallinan
Publikováno v:
Astrophysical Journal; 2/1/2019, Vol. 871 Issue 2, p1-1, 1p