1969
DOI: 10.1007/bf00145519
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The abundance of cadmium in the solar atmosphere

Abstract: The solar spectrum at 3261 & has been studied using the spectrograph at the Oslo Solar Observatory. From analysis of this wavelength region and recent results at 5085 ~, a solar cadmium abundance logNcd = 1.86 4-0.15 is obtained.

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Cited by 6 publications
(2 citation statements)
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“…A breakdown of the standard, grand-canonical ensemble to describe fluctuations of an ideal Bose gas (IBG) and a necessity for canonical or microcanonical description has been noticed long time ago [1], but only in recent decade the problem of fluctuations has received renewed attention due to the experimental achievement of Bose-Einstein condensate (BEC) in ultracold trapped gases. For ideal gases, the canonical and microcanonical fluctuations have been thoroughly investigated [2][3][4][5][6][7][8][9][10], and several powerful techniques, such as the Maxwell Demon ensemble [4,6,7], have been developed.…”
mentioning
confidence: 99%
“…A breakdown of the standard, grand-canonical ensemble to describe fluctuations of an ideal Bose gas (IBG) and a necessity for canonical or microcanonical description has been noticed long time ago [1], but only in recent decade the problem of fluctuations has received renewed attention due to the experimental achievement of Bose-Einstein condensate (BEC) in ultracold trapped gases. For ideal gases, the canonical and microcanonical fluctuations have been thoroughly investigated [2][3][4][5][6][7][8][9][10], and several powerful techniques, such as the Maxwell Demon ensemble [4,6,7], have been developed.…”
mentioning
confidence: 99%
“…To avoid these sorts of unphysically large condensate fluctuations, a canonical (or microcanonical) ensemble has to be used to investigate the fluctuations of the condensate. Within microcanonical and canonical ensembles, the fluctuations of the condensate have been studied in a systematic way in the case of the ideal Bose gas [6][7][8][9][10][11][12][13]. Recently, the question of how interatomic interactions affect the fluctuations of the condensate has been the object of several theoretical investigations [14][15][16][17][18][19].…”
Section: Introductionmentioning
confidence: 99%