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author | Georg Zotti <Georg.Zotti@univie.ac.at> | 2022-03-21 11:27:37 +0100 |
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committer | Georg Zotti <Georg.Zotti@univie.ac.at> | 2022-03-21 11:27:37 +0100 |
commit | 3ddbb7c02672eaefcbff7a82e92fc61a7a622c68 (patch) | |
tree | e436e77886b390866fcfd450ddc8fad545d8e672 | |
parent | d114e453f4e4a2eb37e7aa4be78d0635cd8354aa (diff) |
SUG: Fix bib entry
-rw-r--r-- | guide/ch_astronomical_concepts.tex | 3 | ||||
-rw-r--r-- | guide/guide.bib | 11 |
2 files changed, 11 insertions, 3 deletions
diff --git a/guide/ch_astronomical_concepts.tex b/guide/ch_astronomical_concepts.tex index 59788f3536..ac49637b9d 100644 --- a/guide/ch_astronomical_concepts.tex +++ b/guide/ch_astronomical_concepts.tex @@ -744,7 +744,8 @@ The following list describes sources and a few details about the models for $\De in \citetp{StephensonMorrisonHohenkerk:2016}. The solution combines a spline fit to observations (used between the given limits) with a parabolic fit (used as fallback outside the range, but without smooth transitions at the limits, i.e., - values for 2016 and later deviate notably from current estimates, and should not be used for dates after 2015). The solution was updated in 2021\citetp{StephensonMorrisonHohenkerk:2021}. + values for 2016 and later deviate notably from current estimates, and should not be used for dates after 2015). + The solution was updated in \citetp{StephensonMorrisonHohenkerk:2021}. Recommended range of usage: between years -720.0 and 2019.0 $\dot{n}=-25.82''/\cy^2$. \item[Espenak \& Meeus (2006).] This solution by F. Espenak and J. Meeus, based on diff --git a/guide/guide.bib b/guide/guide.bib index 697165963b..7a28679bc3 100644 --- a/guide/guide.bib +++ b/guide/guide.bib @@ -2018,7 +2018,7 @@ archivePrefix = {arXiv}, @article{StephensonMorrisonHohenkerk:2021, author = {Morrison, L. V. and Stephenson, F. R. and Hohenkerk, C. Y. and Zawilski, M. }, - title = {Addendum 2020 to \&\#x2018;Measurement of the Earth\&\#x2019;s rotation: 720 BC to AD 2015\&\#x2019;}, + title = {Addendum 2020 to `Measurement of the Earth's rotation: 720 BC to AD 2015'}, journal = {Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences}, volume = {477}, number = {2246}, @@ -2027,5 +2027,12 @@ archivePrefix = {arXiv}, doi = {10.1098/rspa.2020.0776}, URL = {https://royalsocietypublishing.org/doi/abs/10.1098/rspa.2020.0776}, eprint = {https://royalsocietypublishing.org/doi/pdf/10.1098/rspa.2020.0776}, - abstract = { Historical reports of solar eclipses are added to our previous dataset (Stephenson et al. 2016 Proc. R. Soc. A 472, 20160404 (doi:10.1098/rspa.2016.0404)) in order to refine our determination of centennial and longer-term changes since 720 BC in the rate of rotation of the Earth. The revised observed deceleration is −4.59 ± 0.08 × 10−22 rad s−2. By comparison the predicted tidal deceleration based on the conservation of angular momentum in the Sun–Earth–Moon system is −6.39 ± 0.03 × 10−22 rad s−2. These signify a mean accelerative component of +1.8 ± 0.1 × 10−22 rad s−2. There is also evidence of an oscillatory variation in the rate with a period of about 14 centuries. } + abstract = { Historical reports of solar eclipses are added to our previous dataset (Stephenson et al. 2016 + Proc. R. Soc. A 472, 20160404 (doi:10.1098/rspa.2016.0404)) in order to refine our + determination of centennial and longer-term changes since 720 BC in the rate of rotation of the + Earth. The revised observed deceleration is −4.59 ± 0.08 × 10−22 rad s−2. By comparison the + predicted tidal deceleration based on the conservation of angular momentum in the + Sun–Earth–Moon system is −6.39 ± 0.03 × 10−22 rad s−2. These signify a mean + accelerative component of +1.8 ± 0.1 × 10−22 rad s−2. There is also evidence + of an oscillatory variation in the rate with a period of about 14 centuries. } } |