summaryrefslogtreecommitdiff
diff options
context:
space:
mode:
authorGeorg Zotti <Georg.Zotti@univie.ac.at>2022-03-21 11:27:37 +0100
committerGeorg Zotti <Georg.Zotti@univie.ac.at>2022-03-21 11:27:37 +0100
commit3ddbb7c02672eaefcbff7a82e92fc61a7a622c68 (patch)
treee436e77886b390866fcfd450ddc8fad545d8e672
parentd114e453f4e4a2eb37e7aa4be78d0635cd8354aa (diff)
SUG: Fix bib entry
-rw-r--r--guide/ch_astronomical_concepts.tex3
-rw-r--r--guide/guide.bib11
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. }
}