Search Publications

Observation of galactic cosmic ray spallation events from the SoHO mission 20-yr operation of LASCO
DOI: 10.1093/mnras/sty1205 Bibcode: 2018MNRAS.478.1265K

Koutchmy, S.; Tavabi, E.; Urtado, O.

A shower of secondary cosmic ray (CR) particles is produced at high altitudes in the Earth's atmosphere, so the primordial galactic cosmic rays (GCRs) are never directly measured outside the Earth magnetosphere and atmosphere. They approach the Earth and other planets in the complex pattern of rigidity's dependence, generally excluded by the magne…

2018 Monthly Notices of the Royal Astronomical Society
SOHO 0
Spectroscopy of Planetary Nebulae with Herschel: A Beginners Guide
DOI: 10.3390/galaxies6030073 Bibcode: 2018Galax...6...73E

Exter, Katrina

A brief overview of the Herschel Space Telescope PACS and SPIRE spectrographs is given, pointing out aspects of working with the data products that should be considered by anyone using them. Some preliminary results of Planetary Nebulae (PNe) taken from the Herschel Planetary Nebula Survey (HerPlaNs) programme are then used to demonstrate what can…

2018 Galaxies
Herschel 0
Results of Photometric and Spectroscopic Observations of the Young Variable Star V730 Cep
DOI: 10.1134/S1063773718120022 Bibcode: 2018AstL...44..798G

Grinin, V. P.; Mkrtichian, D.; Potravnov, I. S. +1 more

We present the results of our photometric ( V RI) and spectroscopic observations of the young variable star V730 Cep (MisV1147) classified by Uemura et al. (2004) as a Herbig Be star. Our photometry confirms the conclusion of the above authors that this star has a complex pattern of variability including periodic or quasi-periodic brightness varia…

2018 Astronomy Letters
Gaia 0
A fresh approach to stellar benchmarking
DOI: 10.1038/d41586-018-05306-7 Bibcode: 2018Natur.558...33B

Beaton, Rachael

An avalanche of data is about to revolutionize astronomy, but the options for validating those data have been limited. High-precision measurements from the Hubble Space Telescope enable a much-needed alternative option.

2018 Nature
Gaia 0
MarsTEM sensor simulations in Martian dust environment
DOI: 10.1016/j.measurement.2017.12.043 Bibcode: 2018Meas..122..453C

Colombatti, Giacomo; Bettanini, Carlo; Aboudan, Alessio +6 more

A wind tunnel test campaign has been conducted prior to the landing of the Exomars2016 EDM module on the Meridiani Planum on the 19th of October 2016. Test were performed in the Mars wind tunnel facility at Aahrus University (DK) under the 2015 Europlanet Call. The facility was available for a 5 days campaign where different environmental configur…

2018 Measurement
ExoMars-16 0
A shear BY field in the Earth's magnetotail and its variations in the current sheet
DOI: 10.1016/j.jastp.2017.08.018 Bibcode: 2018JASTP.177...46G

Malova, Helmi V.; Grigorenko, Elena E.; Zelenyi, Lev M. +2 more

We use Cluster and THEMIS simultaneous observations to study the spatial distributions of a shear BY field in the Plasma Sheet (PS) of the Earth's magnetotail at -31 RE < X < -9 RE. The best correlation between the BY field in the PS (BY_PS) and the Y-component of the Interplanetary Magn…

2018 Journal of Atmospheric and Solar-Terrestrial Physics
Cluster 0
Indirect Detection of Extrasolar Planets via Astrometry
DOI: 10.48550/arXiv.1810.08513 Bibcode: 2018ASPC..517..185B

Matthews, B. C.; Butler, B. J.

Radio wavelength astrometry of stars and other objects has a long and productive history. The use of that technique to determine whether stars have planets around them would cover a nearly unique part of the parameter space for detection of those systems. Namely, astrometric observations are most sensitive to systems with large planets in moderate…

2018 Science with a Next Generation Very Large Array
Gaia 0
The TIRVIM Fourier Spectrometer for Studying the Martian Atmosphere
DOI: 10.1134/S0020441217060070 Bibcode: 2018IET....61..130M

Shakun, A. V.; Moshkin, B. E.; Patsaev, D. V. +3 more

The design and performance features of an IR Fourier-transform spectrometer for studying the Martial atmosphere in the spectrum range of 600-5500 cm-1 during the ExoMars-2016 mission are described. The obtained spectral resolution is in agreement with the theoretical value (0.2 cm-1); the threshold of the instrument sensitivi…

2018 Instruments and Experimental Techniques
ExoMars-16 0
Physics of Partial Ionization in the Solar Chromosphere Revealed by the Solar Optical Telescope Onboard Hinode
DOI: 10.1007/978-981-10-7742-5_19 Bibcode: 2018ASSL..449..211I

Isobe, Hiroaki

2018 First Ten Years of Hinode Solar On-Orbit Observatory
Hinode 0
The Time-Dependent Wavelet Spectrum of HH 1 and 2
Bibcode: 2018RMxAA..54..195R

Raga, A. C.; Esquivel, A.; Riera, A. +2 more

We have calculated the wavelet spectra of four epochs (spanning ≈20 yr) of Hα and [S II] HST images of HH 1 and 2. From these spectra we calculated the distribution functions of the (angular) radii of the emission structures. We found that the size distributions have maxima (corresponding to the characteristic sizes of the observed structures) wit…

2018 Revista Mexicana de Astronomia y Astrofisica
eHST 0