Zobrazeno 1 - 10
of 83
pro vyhledávání: '"Peter Foukal"'
Autor:
Peter Foukal
Publikováno v:
Journal of Astronomical History and Heritage. 24:1059-1062
Autor:
Peter Foukal
Publikováno v:
Physics Today. 75:11-12
Publikováno v:
Journal of Astronomical History and Heritage. 24:1057-1058
Autor:
Peter Foukal
A question posed by a charming Countess sets Philip Frobisher, a Harvard astronomer, on a quest to make a more important contribution to science and society. Anna Grad, a talented Harvard student, interns in Washington for a Senator known for his opp
Autor:
Peter Foukal
Two recent short term dimmings of KIC 8462852 (Boyajian's Star) exhibit clear reddening in the B, r' and i' photometric passbands. We show that the intensity ratios of the three pass bands agree well with cooling of an approximately 6800 K black body
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef09b5b067190df453113d1646dccf0b
Autor:
Peter Foukal
Publikováno v:
Solar Physics. 289:1517-1529
Several studies have shown that the sunspot areas recorded by the Royal Greenwich Observatory (RGO) between 1874 – 1976 are about 40 – 50 % larger than those measured by the NOAA/USAF Solar Observing Optical Network (SOON) since 1966. We show her
Autor:
Peter Foukal
Publikováno v:
Solar Physics. 279:365-381
We compare total solar irradiance (TSI) and ultraviolet (Fuv) irradiance variation reconstructed using Ca K facular areas since 1915, with previous values based on less di- rect proxies. Our annual means for 1925 - 1945 reach values 30 - 50 % higher
Autor:
Peter Foukal, Pietro N. Bernasconi
Publikováno v:
Solar Physics. 248:1-15
Variations in total solar irradiance (TSI) correlate well with changes in projected area of photospheric magnetic flux tubes associated with dark sunspots and bright faculae in active regions and network. This correlation does not, however, rule out
Autor:
Peter Foukal
Area changes of photospheric faculae associated with magnetic active regions are responsible for the bright contribution to variation in total solar irradiance (TSI). Yet, the 102-year white light (WL) facular record measured by the Royal Greenwich O
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a3ff2138a083a75735ac908706245cc7
http://arxiv.org/abs/1505.01040
http://arxiv.org/abs/1505.01040
Publikováno v:
Nature. 443:161-166
Variations in the Sun's total energy output (luminosity) are caused by changing dark (sunspot) and bright structures on the solar disk during the 11-year sunspot cycle. The variations measured from spacecraft since 1978 are too small to have contribu