Zobrazeno 1 - 10
of 253
pro vyhledávání: '"Jeffrey C. Hall"'
Autor:
Evelyne Alecian, C. P. Folsom, Julien Morin, Pascal Petit, Stephen C. Marsden, V. Perdelwitz, M. Mittag, Manuel Guedel, A. Antonova, M. Schmid, Aline A. Vidotto, T. Lüftinger, Y. T. Metodieva, S. Boro Saikia, Sandra V. Jeffers, Jeffrey C. Hall, J.-F. Donati, Oleg Kochukhov
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 658, pp.A16. ⟨10.1051/0004-6361/202141525⟩
Astronomy and Astrophysics
Astronomy & Astrophysics, 658:A16
Astronomy and Astrophysics-A&A, EDP Sciences, In press
HAL
Astronomy and Astrophysics-A&A, 2022, 658, pp.A16. ⟨10.1051/0004-6361/202141525⟩
Astronomy and Astrophysics
Astronomy & Astrophysics, 658:A16
Astronomy and Astrophysics-A&A, EDP Sciences, In press
HAL
A detailed investigation of the magnetic properties of young Sun-like stars can provide valuable information on our Sun's magnetic past and its impact on the early Earth. We determine the properties of the moderately rotating young Sun-like star kapp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8c1e55569375aabd38dd0344a18d892
https://hal.science/hal-03428844/file/2110.06000.pdf
https://hal.science/hal-03428844/file/2110.06000.pdf
Autor:
Aparna Venkatesan, Jeffrey C. Hall, Kelsie Krafton, Joel Parriott, Robert Seaman, Constance E. Walker, Jonathan C. McDowell, Meredith L. Rawls, James D. Lowenthal, Richard F. Green
Publikováno v:
Report of the SATCON2 Workshop, 12–16 July 2021
Autor:
Beate Stelzer, Peter Schneider, Travis S. Metcalfe, Salvatore Orlando, Jorge Sanz-Forcada, M. Mittag, U. Wolter, Jeffrey C. Hall, M. Coffaro, Lorenzo Ducci
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Chromospheric Ca II activity cycles are frequently found in late-type stars, but no systematic programs have been created to search for their coronal X-ray counterparts. The typical time scale of Ca II activity cycles ranges from years to decades. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::655cdf88516f118c941d7215ef6cc0b4
http://hdl.handle.net/10261/233689
http://hdl.handle.net/10261/233689
Autor:
Jeffrey C. Hall
Publikováno v:
Journal of Biological Rhythms. 30:71-75
Earth is the only planet known to harbor life, therefore we may speculate on how the nature of the Sun-Earth interaction is relevant to life on Earth, and how the behavior of other stars may influence the development of life on their planetary system
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f054b0db786aa9b1380d46f7fd4f36e
http://arxiv.org/abs/1704.02388
http://arxiv.org/abs/1704.02388
Autor:
Ricky Egeland, Alexei A. Pevtsov, S. L. Baliunas, Jeffrey C. Hall, Luca Bertello, Willie Soon
The most commonly used index of stellar magnetic activity is the instrumental flux scale of singly-ionized calcium H & K line core emission, S, developed by the Mount Wilson Observatory (MWO) HK Project, or the derivative index R'_HK. Accurately plac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::67f32e60ea4a59304b529807d5e08a31
http://urn.fi/urn:nbn:fi-fe201903057198
http://urn.fi/urn:nbn:fi-fe201903057198
Autor:
C. P. Folsom, Jeffrey C. Hall, Robert H. Cameron, Ansgar Reiners, Sandra V. Jeffers, Stephen C. Marsden, Aline A. Vidotto, Julien Morin, Pascal Petit, J.-F. Donati, S. Boro Saikia, V. Perdelwitz
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 594, pp.A29. ⟨10.1051/0004-6361/201628262⟩
NASA Astrophysics Data System
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 594, pp.A29. ⟨10.1051/0004-6361/201628262⟩
NASA Astrophysics Data System
International audience; The long-term monitoring of magnetic cycles in cool stars is a key diagnostic in understanding how dynamo generation and amplification of magnetic fields occur in stars similar in structure to the Sun. We investigate the tempo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db503b19c75b2dd155c53a01bf1bedb2
https://hal.archives-ouvertes.fr/hal-01529718
https://hal.archives-ouvertes.fr/hal-01529718
Publikováno v:
The Astrophysical Journal. 855:75
Publikováno v:
The Astronomical Journal. 138:312-322
We present 14 years of contemporaneous photometric and spectroscopic observations of 28 solar analog stars, taken with the Tennessee State University Automatic Photometric Telescopes at Fairborn Observatory and the Solar-Stellar Spectrograph at Lowel
Autor:
Jeffrey C. Hall, F. Favata, Salvatore Orlando, Salvatore Sciortino, J. H. M. M. Schmitt, Giuseppina Micela
Publikováno v:
Astronomy & Astrophysics. 490:1121-1126
(abridged) Our long-term XMM-Newton program of long-term monitoring of a solar-like star with a well-studied chromospheric cycle, HD 81809 aims to study whether an X-ray cycle is present, along with studying its characteristics and its relation to th