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pro vyhledávání: '"Solar transit"'
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Autor:
Hebbeker, Thomas
Asteroid transits across the Sun are predicted for the years 2023 till 2040. None of them can be detected from Earth.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20b3339b6b0b96f7bf0404726812256a
Autor:
Reza Akbar
Publikováno v:
Al-Marshad: Jurnal Astronomi Islam dan Ilmu-Ilmu Berkaitan. 5:192-204
The shadow less phenomenon in a city is actually already known by the people in Indonesia. In the City of Sambas, the shadow less phenomenon has not been as popular as in the City of Pontianak. The public perception in general is that phenomenon does
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c94c166e60d3e51c205fce3c89f68a7e
https://doi.org/10.30596/jam.v5i2.3555
https://doi.org/10.30596/jam.v5i2.3555
Publikováno v:
Journal of Guidance, Control, and Dynamics. 38:489-505
Designs for geostationary solar power satellites are extremely large in scale, more than an order of magnitude larger than the International Space Station. A detailed study of solar power satellites’ orbit dynamics is performed, obtaining a compreh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e9952bfede950869796c1566601da6b4
https://doi.org/10.2514/1.g000609
https://doi.org/10.2514/1.g000609
The May 9, 2016, transit of Mercury was observed simultaneously from the Big Bear Solar Observatory in California and from a site in Germany. From the measured displacement between the views from the two sites of Mercury’s disk silhouetted against
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f96f48e68ac3a035eda41428f982be2
https://resolver.caltech.edu/CaltechAUTHORS:20170616-160918081
https://resolver.caltech.edu/CaltechAUTHORS:20170616-160918081
Publikováno v:
2016 IEEE International Autumn Meeting on Power, Electronics and Computing (ROPEC).
The efficient generation of renewable energy coming from a solar system depends strongly on the direction at which the sun rays strike the surface of the solar collector. Therefore, the knowledge at any time of the sun position is very important for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::afe6297a845f224ed0bdfe208b293abc
https://doi.org/10.1109/ropec.2016.7830580
https://doi.org/10.1109/ropec.2016.7830580
Autor:
René Heller, Ralph E. Pudritz
Publikováno v:
Astrobiology. 16(4)
Over the past few years, astronomers have detected thousands of planets and candidate planets by observing their periodic transits in front of their host stars. Related methods might soon allow studies of the chemical imprints of life in extrasolar p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::214353ee53356bd10f82ed6be8763204
https://pubmed.ncbi.nlm.nih.gov/26967201
https://pubmed.ncbi.nlm.nih.gov/26967201
Autor:
Costantino Sigismondi
Publikováno v:
International Journal of Modern Physics: Conference Series. 12:229-236
A sunset over the sea surface offers the possibility to chronometrate a solar transit across the horizon. The vertical solar diameter is proportional to the duration of the sunset, the cosine of the azimuth and the cosine of the latitude of the obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c5644c35e971266fc52a36017eb8971
https://doi.org/10.1142/s2010194512006423
https://doi.org/10.1142/s2010194512006423
Autor:
V. S. Kotel’nikov, P. G. Tsybulev, N. A. Nizhel’skij, O. A. Golubchina, G. N. Zhekanis, A. N. Korzhavin, V. M. Bogod
Publikováno v:
Astrophysical Bulletin. 62:360-368
We report the results of unique observations of the solar eclipse of March 29, 2006 over a wide radio-wavelength range from 1 to 50 cm made with the large RATAN-600 stationary radio telescope during the maximum eclipse phase performed using the metho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8f0552c7bba46098c16caaddbaf0b23f
https://doi.org/10.1134/s1990341307040074
https://doi.org/10.1134/s1990341307040074
Doppler shifts of sub-millimeter 12 CO (346 GHz) and 13 CO (330 GHz) and millimeter 12 CO (230 GHz) line absorptions were mapped around the circum-disk terminator of Venus before, during, and after the June 5, 2012 solar transit, employing the James
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da9ed98baa2bc643f18afa39dc1803a6
https://doi.org/10.1016/j.icarus.2015.03.031
https://doi.org/10.1016/j.icarus.2015.03.031