As digital technology becomes more prevalent in today’s business environment and interest in digital trust rises, restaurants need to identify whether and how their mobile apps enhance the customer experience, and what features of the apps can strengthen customers’ attachment to them. However, few studies have examined the role of restaurant mobile apps as a catalyst for building customer loyalty. Considering restaurant mobile apps as a means to build a trustworthy relationship between customers and restaurants, this study develops and validates a research framework to measure digital trust between restaurants and customers through restaurant mobile apps. Specifically, due to the lack of measurement constructs for digital trust, a reliable and valid set of measurements that can explain digital trust in relation to restaurant mobile apps is developed and the effects of mobile apps’ digital trust on customers’ trust in a restaurant brand, overall experience, and their continued use intention are assessed.

The fall armyworm (FAW), Spodoptera frugiperda J.E. Smith is a noctuid moth endemic throughout the Western Hemisphere that has recently become widespread in sub-Saharan Africa. In Asia, FAW was firstly reported at corn fields in India, SriLanka, Bangladeshi, Miyanmar and Thailand in 2018. In January 2019, FAW was also found in Yunnan province of China. In March 2019, the larvae which could be tentatively identified as FAW were caught at a corn field of Plant Protection Center of Lao PDR, which is located in Vientiane, Laos. Species identification was confirmed by DNA barcoding using the COⅠ segment of the four larvae, which were found to be the haplotype of rice strain (COⅠ-RS). The host strain identity was additionally analysed as a Tpi-C (C-strain allele) by Triosephosphate isomerase gene (Tpi) segment located on the Z sex chromosome. The result shows that the FAW specimens in Lao is the subpopulation of COⅠ-RS/Tpi-C (COⅠ and Tpi haplotype combination). It was reported that COⅠ-CS/Tpi-C were more frequently observed than COⅠ-RS/Tpi-C in Western Hemisphere and Western Africa, but COⅠ-RS/Tpi-C were more frequently observed in Eastern Africa. It can be supposed that the subpopulation of COⅠ-RS/Tpi-C in Lao is one of the subpopulations which have migrated into the Indochinese peninsula from Eastern Africa, with more detailed analysis for more diverse nationwide specimens left.

We investigate two abnormal CME-Storm pairs that occurred on 2014 September 10 - 12 and 2015 March 15 - 17, respectively. The first one was a moderate geomagnetic storm (Dstmin  -75 nT) driven by the X1.6 high speed flare-associated CME (1267 km s−1) in AR 12158 (N14E02) near solar disk center. The other was a very intense geomagnetic storm (Dstmin  -223 nT) caused by a CME with moderate speed (719 km s−1) and associated with a filament eruption accompanied by a weak flare (C9.1) in AR 12297 (S17W38). Both CMEs have large direction parameters facing the Earth and southward magnetic field orientation in their solar source region. In this study, we inspect the structure of Interplanetary Flux Ropes (IFRs) at the Earth estimated by using the torus fitting technique assuming self-similar expansion. As results, we find that the moderate storm on 2014 September 12 was caused by small-scale southward magnetic fields in the sheath region ahead of the IFR. The Earth traversed the portion of the IFR where only the northward fields are observed. Meanwhile, in case of the 2015 March 17 storm, our IFR analysis revealed that the Earth passed the very portion where only the southward magnetic fields are observed throughout the passage. The resultant southward magnetic field with long- duration is the main cause of the intense storm. We suggest that 3D magnetic field geometry of an IFR at the IFR-Earth encounter is important and the strength of a geomagnetic storm is strongly affected by the relative location of the Earth with respect to the IFR structure.

Leptotrombidium pallidum is the major vector mites for Orientia tsutsugamushi, the causative agent of scrub typhus. To understand the molecular mechanism of L. pallidum, we sequenced the whole genome using Illumina sequencing technology. Totally four genomic libraries with different insert sizes ranging from 280 bp to 8 kb were used to generate 45.1 Gb of genome in the combination of paired-end and mate-pairs sequencing reads. Quality filtering and correction of paired-end reads for very small and/or bad-quality sequences yielded 26.9 Gb of high-quality sequences, which are used to estimate the genome size as 175 Mbusing kmer methods and assembled into a 193.7 Mb genomic sequence scaffolds with N50 length of 92,945 bp. Furthermore, 94% of CEGMA completeness score were obtained from genome scaffold assembly. To facilitate gene annotation, we used a combination of de novo and homology based tools to predict gene models in the chigger mite genome. A combination of evidence-based and de novo approaches predicted 15,842 high-confidence protein-coding genes with an average transcript length of 1,511 bp and 2.4 exons per gene which corresponds to about 12.4% total gene length. Bacterial endosymbiosis are very common in mite species and can range from mutualistic to pathogenic associations. Henceforth, the endosymbionts in L. pallidum were predicted using the NCBI microbial draft genomes and mitochondrial genome. Besides, this L. pallidum draft genome can be used as a significant reference for comparative genomic studies across mite species.

We present BV CCD photometry for the open clusters Czernik 24 and Czernik 27. These clusters have never been studied before, and we provide, for the first time, the cluster parameters; reddening, distance, metallicity and age. Czernik 24 is an old open cluster with age 1.8 ± 0.2 Gyr, metallicity [Fe/H]=-0.41 ± 0.15 dex, distance modulus (m-M)0=13.1 ± 0.3 mag (d=4.1 ± 0.5 kpc), and reddening E(B-V)=0.54 ± 0.12 mag. The parameters for Czernik 27 are estimated to be age=0.63 ± 0.07 Gyr, [Fe/H]=-0.02 ± 0.10 dex, (m-M)0=13.8 ± 0.2 mag (d=5.8 ± 0.5 kpc), and E(B-V)=0.15 ± 0.05 mag. The metallicity and distance values for Czernik 24 are consistent with the relation between the metallicity and the Galactocentric distance of other old open clusters. We find the metallicity gradient of 51 old open clusters including Czernik 24 to be Δ[Fe/H]/ΔRgc = -0.064±0.009 dex kpc-1.