scholarly journals Preliminary results of a Taimyr-Evenk reindeer population study using the Argos/GPS satellite system in 2015-2016

Author(s):  
A P Savchenko ◽  
I A Savchenko ◽  
P A Savchenko ◽  
S A Dubintsov ◽  
N V Karpova ◽  
...  
2011 ◽  
Vol 29 ◽  
pp. e17
Author(s):  
M. T. Bonati ◽  
M. C. Monti ◽  
C. Crocamo ◽  
C. Montomoli ◽  
O. Terradura-Vagnarelli ◽  
...  

1993 ◽  
Vol 16 (5) ◽  
pp. 515-538 ◽  
Author(s):  
C. Bonifazi ◽  
G. Manarini ◽  
J. Sabbagh ◽  
F. Svelto ◽  
D. C. Thompson ◽  
...  

2019 ◽  
Vol 11 (24) ◽  
pp. 3013 ◽  
Author(s):  
Cheng Jing ◽  
Xinliang Niu ◽  
Chongdi Duan ◽  
Feng Lu ◽  
Guodong Di ◽  
...  

Launched on 5 June 2019, the BuFeng-1 A/B twin satellites were part of the first Chinese global navigation satellite system reflectometry (GNSS-R) satellite mission. In this letter, a brief introduction of the BF-1 mission and its preliminary results of sea surface wind retrieval are presented. Empirical fully developed sea (FDS) geophysical model functions (GMFs) relating the normalized bistatic radar cross-section to the sea surface wind speed are proposed for the BF-1 GNSS-R instruments. The FDS GMFs are derived from the collocated BF-1 observations, the European Center for Medium-Range Weather Forecasts (ECMWF) reanalysis data, and the advanced scatterometer (ASCAT) satellite observations. The preliminary tests reveal that the root-mean-square error (RMSE) between the derived wind speed and the reanalysis is 2.63 m/s for wind speeds in the range of 0.5–40.5 m/s. Further comparisons with the ASCAT observations and mooring buoys show that the RMSEs are 2.04 m/s and 1.77 m/s, respectively, at low-to-moderate wind speeds. This study demonstrates the effectiveness of BF-1 and provides a basis for the future GMF development of the BF-1 A/B mission.


2015 ◽  
Vol 53 (10) ◽  
pp. 5760-5773 ◽  
Author(s):  
Tao Zeng ◽  
Dongyang Ao ◽  
Cheng Hu ◽  
Tian Zhang ◽  
Feifeng Liu ◽  
...  

2012 ◽  
Vol 33 (S1) ◽  
pp. 87-90 ◽  
Author(s):  
F. Moschiano ◽  
P. Messina ◽  
D. D’Amico ◽  
L. Grazzi ◽  
F. Frediani ◽  
...  

2012 ◽  
Vol 18 (5(78)) ◽  
pp. 59-65 ◽  
Author(s):  
M.A. Popov ◽  
S.A. Stankevich ◽  
Y.I. Zyelyk ◽  
S.V. Shklyar ◽  
O.V. Semeniv ◽  
...  

Thorax ◽  
2010 ◽  
Vol 65 (Suppl 4) ◽  
pp. A129-A129 ◽  
Author(s):  
R. Mukherjee ◽  
V. C. Moore ◽  
S. Purkait ◽  
P. Goon ◽  
C. J. Warburton ◽  
...  

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


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