Variability in the Astronomical Refraction of the Rising and Setting Sun
Observed timings of 244 sunrises and 135 sunsets from two closely spaced geographic locations in Edmonton, Alberta, were used to determine astronomical refraction for the Sun’s upper limb. The observed astronomical refraction had a mean of 0 \documentclass{aastex} \usepackage{amsbsy} \usepackage{ams...
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| Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 2003-10, Vol.115 (812), p.1256-1261 |
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| container_title | Publications of the Astronomical Society of the Pacific |
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| creator | Sampson, Russell D. Lozowski, Edward P. Peterson, Arthur E. Hube, Douglas P. |
| description | Observed timings of 244 sunrises and 135 sunsets from two closely spaced geographic locations in Edmonton, Alberta, were used to determine astronomical refraction for the Sun’s upper limb. The observed astronomical refraction had a mean of 0
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669, a standard deviation of 0
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175, and a range between 0
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402 and 2
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| doi_str_mv | 10.1086/378214 |
| format | Article |
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669, a standard deviation of 0
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175, and a range between 0
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402 and 2
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081. At sunrise, the astronomical refraction had a mean of 0
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714, a standard deviation of 0
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184, and a range between 0
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402 and 2
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081. At sunset, the astronomical refraction had a mean of 0
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579, a standard deviation of 0
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108, and a range between 0
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442 and 1
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085. There is a strong annual variation of the monthly mean and the monthly standard deviation of the astronomical refraction. Both parameters reach a maximum during the coldest months for sunrises and sunsets. Abnormally large refraction events—sometimes called Novaya Zemlya solar mirages—can occur in both warm and cold months.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/378214</identifier><language>eng</language><publisher>The University of Chicago Press</publisher><subject>Altitude ; Archaeoastronomy ; Astronomical research ; Astronomy ; Climate models ; Geodetic position ; Horizon coordinate system ; Observational astronomy ; Refraction ; Standard deviation</subject><ispartof>Publications of the Astronomical Society of the Pacific, 2003-10, Vol.115 (812), p.1256-1261</ispartof><rights>2003. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c281t-40cff0cdb84143ef95a68df4ed711728b7a4c1ec22c6757d7d6bb0db743ee0373</citedby><cites>FETCH-LOGICAL-c281t-40cff0cdb84143ef95a68df4ed711728b7a4c1ec22c6757d7d6bb0db743ee0373</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,799,27901,27902</link.rule.ids></links><search><creatorcontrib>Sampson, Russell D.</creatorcontrib><creatorcontrib>Lozowski, Edward P.</creatorcontrib><creatorcontrib>Peterson, Arthur E.</creatorcontrib><creatorcontrib>Hube, Douglas P.</creatorcontrib><title>Variability in the Astronomical Refraction of the Rising and Setting Sun</title><title>Publications of the Astronomical Society of the Pacific</title><description>Observed timings of 244 sunrises and 135 sunsets from two closely spaced geographic locations in Edmonton, Alberta, were used to determine astronomical refraction for the Sun’s upper limb. The observed astronomical refraction had a mean of 0
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669, a standard deviation of 0
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175, and a range between 0
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402 and 2
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081. At sunrise, the astronomical refraction had a mean of 0
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714, a standard deviation of 0
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184, and a range between 0
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402 and 2
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081. At sunset, the astronomical refraction had a mean of 0
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579, a standard deviation of 0
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108, and a range between 0
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442 and 1
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085. There is a strong annual variation of the monthly mean and the monthly standard deviation of the astronomical refraction. Both parameters reach a maximum during the coldest months for sunrises and sunsets. Abnormally large refraction events—sometimes called Novaya Zemlya solar mirages—can occur in both warm and cold months.</description><subject>Altitude</subject><subject>Archaeoastronomy</subject><subject>Astronomical research</subject><subject>Astronomy</subject><subject>Climate models</subject><subject>Geodetic position</subject><subject>Horizon coordinate system</subject><subject>Observational astronomy</subject><subject>Refraction</subject><subject>Standard deviation</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><recordid>eNp1j01LAzEURYMoWKv-hoDgbvS9SWYSl6VoKxSEVt0O-dSUaUaSuOi_t3XcuroX7uHCIeQa4Q5BtvdMyBr5CZlgw2TFpGCnZAIAvGprCefkIuctAKJEmJDlu0pB6dCHsqch0vLp6CyXNMRhF4zq6dr5pEwJQ6SD_53XIYf4QVW0dONKOfbNd7wkZ1712V395ZS8PT2-zpfV6mXxPJ-tKlNLLBUH4z0YqyVHzpx_aFQrrefOCkRRSy0UN-hMXZtWNMIK22oNVosD7IAJNiW3469JQ87J-e4rhZ1K-w6hO_p3o_8BvBnBbS5D-o_6AYJBV8U</recordid><startdate>200310</startdate><enddate>200310</enddate><creator>Sampson, Russell D.</creator><creator>Lozowski, Edward P.</creator><creator>Peterson, Arthur E.</creator><creator>Hube, Douglas P.</creator><general>The University of Chicago Press</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>200310</creationdate><title>Variability in the Astronomical Refraction of the Rising and Setting Sun</title><author>Sampson, Russell D. ; Lozowski, Edward P. ; Peterson, Arthur E. ; Hube, Douglas P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c281t-40cff0cdb84143ef95a68df4ed711728b7a4c1ec22c6757d7d6bb0db743ee0373</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2003</creationdate><topic>Altitude</topic><topic>Archaeoastronomy</topic><topic>Astronomical research</topic><topic>Astronomy</topic><topic>Climate models</topic><topic>Geodetic position</topic><topic>Horizon coordinate system</topic><topic>Observational astronomy</topic><topic>Refraction</topic><topic>Standard deviation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sampson, Russell D.</creatorcontrib><creatorcontrib>Lozowski, Edward P.</creatorcontrib><creatorcontrib>Peterson, Arthur E.</creatorcontrib><creatorcontrib>Hube, Douglas P.</creatorcontrib><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sampson, Russell D.</au><au>Lozowski, Edward P.</au><au>Peterson, Arthur E.</au><au>Hube, Douglas P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Variability in the Astronomical Refraction of the Rising and Setting Sun</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>2003-10</date><risdate>2003</risdate><volume>115</volume><issue>812</issue><spage>1256</spage><epage>1261</epage><pages>1256-1261</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>Observed timings of 244 sunrises and 135 sunsets from two closely spaced geographic locations in Edmonton, Alberta, were used to determine astronomical refraction for the Sun’s upper limb. The observed astronomical refraction had a mean of 0
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669, a standard deviation of 0
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175, and a range between 0
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402 and 2
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081. At sunrise, the astronomical refraction had a mean of 0
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714, a standard deviation of 0
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184, and a range between 0
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402 and 2
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081. At sunset, the astronomical refraction had a mean of 0
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579, a standard deviation of 0
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108, and a range between 0
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442 and 1
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085. There is a strong annual variation of the monthly mean and the monthly standard deviation of the astronomical refraction. Both parameters reach a maximum during the coldest months for sunrises and sunsets. Abnormally large refraction events—sometimes called Novaya Zemlya solar mirages—can occur in both warm and cold months.</abstract><pub>The University of Chicago Press</pub><doi>10.1086/378214</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-6280 |
| ispartof | Publications of the Astronomical Society of the Pacific, 2003-10, Vol.115 (812), p.1256-1261 |
| issn | 0004-6280 1538-3873 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_378214 |
| source | Jstor Complete Legacy; IOP Publishing Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection |
| subjects | Altitude Archaeoastronomy Astronomical research Astronomy Climate models Geodetic position Horizon coordinate system Observational astronomy Refraction Standard deviation |
| title | Variability in the Astronomical Refraction of the Rising and Setting Sun |
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