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The close encounter of Comet C/2013 A1 (Siding Spring) with Mars on October 19, 2014 presented an extremely rare opportunity to obtain the first flyby quality data of the nucleus and inner coma of a dynamically new comet. However, the…

The onset of the "Rush to the Poles" of polar-crown prominences and their associated coronal emission is a harbinger of solar maximum. Altrock (Solar Phys. 216, 343, 2003) showed that the "Rush" was well-observed at 1.15 Ro in the Fe XIV…

Solar and Stellar Astrophysics · Physics 2013-02-22 Richard C. Altrock

This paper presents CI, CO J=4-3, and CO J=3-2 maps of the barred spiral galaxy M83 taken at the James Clerk Maxwell Telescope. Observations indicate a double peaked structure which is consistent with gas inflow along the bar collecting at…

Astrophysics · Physics 2009-10-30 Glen R. Petitpas , Christine D. Wilson

Understanding coronal structure and dynamics can be facilitated by analyzing green-line emission, which enables the investigation of diverse coronal structures such as coronal loops, streamers, coronal holes, and various eruptions in the…

Solar and Stellar Astrophysics · Physics 2024-11-27 Jacob Oloketuyi , Yu Liu , Linhua Deng , Abouazza Elmhamdi , Fengrong Zhu , Ayodeji Ibitoye , Opeyemi Omole , Feiyang Sha , Qiang Liu

Recent observations indicate potentially carbon-rich exoplanet atmospheres. Spectral fitting methods for brown dwarfs and exoplanets have invoked the C/O ratio as additional parameter but carbon-rich cloud formation modeling is a challenge…

Solar and Stellar Astrophysics · Physics 2021-06-04 Ch. Helling , D. Tootill , P. Woitke , E. K. H. Lee

The 11-year solar cycle is the dominant pattern of solar activity reflecting the oscillatory dynamo mechanism in the Sun. Solar cycles were directly observed since 1700, while indirect proxies suggest their existence over a much longer…

Solar and Stellar Astrophysics · Physics 2021-03-30 I. G. Usoskin , S. K. Solanki , N. Krivova , B. Hofer , G. A. Kovaltsov , L. Wacker , N. Brehm , B. Kromer

Hadronic jets are extremely abundant at the LHC, and testing QCD in various corners of phase-space is important to understand backgrounds and some specific signatures of new physics. In this article, various measurements aiming at probing…

High Energy Physics - Phenomenology · Physics 2015-08-20 Mario Campanelli

The solar activity in Cycle 23--24 shows differences from the previous cycles that were observed with modern instruments, e.g. long cycle duration and a small number of sunspots. To appreciate the anomalies further, we investigated the…

Solar and Stellar Astrophysics · Physics 2015-06-16 Masumi Shimojo

There is a deep cosmological mystery: although dependent on very different underlying physics, the timescales of structure formation, of galaxy cooling (both radiatively and against the CMB), and of vacuum domination do not differ by many…

High Energy Physics - Theory · Physics 2009-09-24 Raphael Bousso , Lawrence J. Hall , Yasunori Nomura

In this paper, we present a unique data set of more than one year's worth of regular observations of comet C/2013 A1(Siding Spring) with TRAPPIST in Chile, along with low-resolution spectra obtained with the ESO/VLT FORS 2 instrument. The…

Earth and Planetary Astrophysics · Physics 2016-04-20 C. Opitom , A. Guilbert-Lepoutre , E. Jehin , J. Manfroid , D. Hutsemékers , M. Gillon , P. Magain , G. Roberts-Borsani , O. Witasse

The experimental data on continuous investigation of changes in beta-decay count rate of Cs-137 and Co-60 from 9.12.98 till 30.04.99, are presented. The 27-day and 24-hour periods in these changes, inexplicable by traditional physics, have…

High Energy Physics - Experiment · Physics 2007-05-23 Yu. A. Baurov , Yu. G. Sobolev , V. F. Kushniruk , A. N. Kuznetzov , A. A. Konradov

Recent work has revealed a 62 (+/-) 3-million-year cycle in the fossil diversity in the past 542 My, however no plausible mechanism has been found. We propose that the cycle may be caused by modulation of cosmic ray (CR) flux by the Solar…

Astrophysics · Physics 2008-11-26 Mikhail V. Medvedev , Adrian L. Melott

Increases in atmospheric CO2 and CH4 result from a combination of forcing from anthropogenic emissions and Earth System feedbacks that reduce or amplify the effects of those emissions on atmospheric concentrations. Despite decades of…

We show fifty-seven enhanced radiation level events taken from new measurements on commercial altitude (greater than 9 km) aircraft that are analogous to planes flying through radiation clouds. More accurately, the plane is likely to be…

Space Physics · Physics 2022-09-14 W. Kent Tobiska , Alexa J. Halford , Steven K. Morley

Magnetic reconnection is thought to be a key process in most of solar eruptions. Thanks to high-resolution observations and simulations, the studied scale of reconnection process has become smaller and smaller. Spectroscopic observations…

Solar and Stellar Astrophysics · Physics 2019-05-15 Dong Li

Recent large-area, deep CO surveys in the Galactic disk have revealed the formation of ~50 high-mass stars or clusters triggered by cloud-cloud collisions (CCCs). Although the Galactic Center (GC) -- which contains the highest volume…

Astrophysics of Galaxies · Physics 2020-01-08 Rei Enokiya , Kazufumi Torii , Yasuo Fukui

Models of thermal evolution, crustal production, and CO$_2$ cycling are used to constrain the prospects for habitability of rocky planets, with Earth-like size and composition, in the stagnant lid regime. Specifically, we determine the…

Earth and Planetary Astrophysics · Physics 2018-07-25 Bradford J. Foley , Andrew J. Smye

Comet C/2013 A1 (siding Spring) will experience a high velocity encounter with Mars on October 19, 2014 at a distance of 135,000 km +- 5000 km from the planet center. We present a comprehensive analysis of the trajectory of both the comet…

Earth and Planetary Astrophysics · Physics 2015-06-19 Davide Farnocchia , Steven R. Chesley , Paul W. Chodas , Pasquale Tricarico , Michael S. P. Kelley , Tony L. Farnham

We have observed several emission lines of two Nitrogen-bearing (C2H5CN and C2H3CN) and two Oxygen-bearing (CH3OCH3 and HCOOCH3) molecules towards a sample of well-known hot molecular cores (HMCs) in order to check whether the chemical…

Astrophysics · Physics 2009-11-13 F. Fontani , I. Pascucci , P. Caselli , F. Wyrowski , R. Cesaroni , C. M. Walmsley