Search Publications

Brief Communication: The double layer in the separatrix region during magnetic reconnection
DOI: 10.5194/npg-22-167-2015 Bibcode: 2015NPGeo..22..167G

Guo, J.; Yu, B.

With two-dimensional (2-D) particle-in-cell (PIC) simulations we investigate the evolution of the double layer (DL) driven by magnetic reconnection. Our results show that an electron beam can be generated in the separatrix region as magnetic reconnection proceeds. This electron beam could trigger the ion-acoustic instability; as a result, a DL acc…

2015 Nonlinear Processes in Geophysics
Cluster 0
Lunar absolute reflectance as observed by Chang'E-1 Imaging Interferometer
DOI: 10.1007/s11433-015-5680-9 Bibcode: 2015SCPMA..58.9601Z

Li, Bo; Zhang, Jiang; Ling, ZongCheng +3 more

Lunar absolute reflectance, which describes the fraction of solar radiation reflected by the Moon, is fundamental for the Chang'E-1 Imaging Interferometer (IIM) to map lunar mineralogical and elemental distributions. Recent observations made by the Spectral Irradiance Monitor (SIM) onboard the Solar Radiation and Climate Experiment (SORCE) spacecr…

2015 Science China Physics, Mechanics, and Astronomy
Chandrayaan-1 0
Rosetta's comet is rich in deuterium
DOI: 10.1063/PT.3.2675 Bibcode: 2015PhT....68b..16W

Wilson, R. Mark

2015 Physics Today
Rosetta 0
Comets are Nice to Touch
DOI: 10.1007/BF03404702 Bibcode: 2015AeMiS..94..210F

Finzi, A. Ercoli

Rosetta is the third cornerstone mission of the European Space Agency scientific program "Horizon 2000" and it is the first spacecraft to orbit around a comet nucleus and to send a lander on its surface with the aim of studying the real nature of these objects. It was launched in March 2004 and reached the comet 67P/Churymov-Gerasimenko in 2014. I…

2015 Aerotecnica Missili & Spazio
Rosetta 0
Philae mission set for reboot
DOI: 10.1088/2058-7058/28/5/12 Bibcode: 2015PhyW...28e...7B

Banks, Michael

Scientists at the European Space Agency (ESA) are hoping that the Philae lander, which successfully landed on a comet last year, will re-establish contact soon as it travels closer to the Sun.

2015 Physics World
Rosetta 0
Philae set for science after waking up from hibernation
DOI: 10.1088/2058-7058/28/7/11 Bibcode: 2015PhyW...28a...7B

Banks, Michael

The European Space Agency's Philae lander has woken up following seven months in hibernation mode.

2015 Physics World
Rosetta 0
Rosetta Studies of Comet 67P/Churyumov-Gerasimenko: Prospects for Establishing Cometary Biology
DOI: 10.4172/2332-2519.1000126 Bibcode: 2015JAsBO...3..126S

Smith, W. E.; Wainwright, M.

2015 Journal of Astrobiology & Outreach
Rosetta 0
An AKARI infrared study of dust emission in Galactic bubbles indicative of large-scale cloud-cloud collisions
DOI: 10.1016/j.pss.2015.04.006 Bibcode: 2015P&SS..116...57H

Kaneda, H.; Sano, H.; Ishihara, D. +3 more

We report our systematic study on dust emission in massive star-forming regions indicative of large-scale cloud-cloud collisions, using the AKARI infrared (IR) all-sky survey data at wavelengths of 9, 18, 65, 90, 140, and 160 µm. We focus on the Galactic bubbles catalogued by Spitzer, which are categorized into two types of morphology, close…

2015 Planetary and Space Science
AKARI 0
Identification of Luminous White Dwarf Candidates in the Globular Clusters M13 and M22 Using HST Acs Photometric Data
DOI: 10.5303/PKAS.2015.30.2.265 Bibcode: 2015PKAS...30..265C

CHO, DONG-HWAN; YOON, TAE SEOG; LEE, SANG-GAK +1 more

2015 Publication of Korean Astronomical Society
eHST 0
The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
DOI: 10.17721/2227-1481.5.79-83 Bibcode: 2015AASP....5...79S

Tugay, A. V.; Sadova, V. A.

X-ray luminosities and spectral indices of 97 bright Seyfert 1 (Sy1) galaxies from the XMM-Newton archive are analysed in this article. Distribution of these values is random, so we conclude that the model of emission should be at least two-parametric. Within the framework of the merging model of active galactic nuclei (AGN), the relation between …

2015 Advances in Astronomy and Space Physics
XMM-Newton 0