scholarly journals The Impact of the COVID-19 Pandemic on Scientific Publishing

2021 ◽  
Vol 22 (3) ◽  
pp. 484-488
Author(s):  
Philip D. Sloane ◽  
Sheryl Zimmerman
Keyword(s):  
Scientific Publishing ◽  
The Impact

scholarly journals Data Sharing Policies: Share Well and You Shall be Rewarded

2021 ◽  
Author(s):  
Jean Peccoud
Keyword(s):  
Data Sharing ◽  
Scientific Community ◽  
Computer Software ◽  
Research Data ◽  
Objective Data ◽  
Scientific Publishing ◽  
Publishing Process ◽  
Administrative Burden ◽  
Textual Description ◽  
The Impact

Abstract Sharing research data is an integral part of the scientific publishing process. By sharing data authors enable their readers to use their results in a way that the textual description of the results does not allow by itself. In order to achieve this objective, data should be shared in a way that makes it as easy as possible for readers to import them in computer software where they can be viewed, manipulated, and analyzed. Many authors and reviewers seem to misunderstand the purpose of the data sharing policies developed by journals. Rather than being an administrative burden that authors should comply with to get published, the objective of these policies is to help authors maximize the impact of their work by allowing other members of the scientific community to build upon it. Authors and reviewers need to understand the purpose of data sharing policies to assist editors and publishers in their efforts to ensure that every article published complies with them.

scholarly journals Toward a Sustainable Model of Scientific Publishing

2021 ◽  
Vol 18 (01) ◽  
Author(s):  
Ravindra Palavalli-Nettimi
Keyword(s):  
Value Added ◽  
Academic Publishing ◽  
Scientific Publishing ◽  
Budget Cuts ◽  
Research Papers ◽  
Journal Publication ◽  
The Public ◽  
Funding Sources ◽  
Open Access Journals ◽  
The Impact

The current models of commercial publishing of scientific research costs universities, funding organizations, and governments billions of dollars in the form of annual subscriptions and publishing charges. Yet, many research papers are behind a paywall for the public and those unaffiliated to universities. Much of the research that is freely accessible to everyone requires authors to pay an unreasonable fee leading to inequalities in knowledge dissemination based on affordability. So, we need a sustainable model of scientific publishing that is beneficial to scientists, universities, and the public, especially in light of Covid-19 pandemic related budget cuts. Similar to commercial publishers, many scientific societies publish their own journals. Funding sources and universities should offer publishing grants or annual contributions to fund such societies’ open-access journals and thus support a sustainable publishing model wherein profits generated from academic publishing are invested back into the scientific community. Funding sources should also mandate publishing papers in society journals. To encourage that, hiring committees should place more importance on the article-level metrics than journal quality metrics such as the impact factor. The societies can use the publishing grants to cover journal publication costs and pay commercial publishers only for their value-added services such as manuscript handling and hosting the content online. The proposed publishing model will be sustainable and can strengthen scientific communities by supporting scientific society journals and making science more accessible.

scholarly journals The impact of COVID-19 on scientific publishing

2020 ◽  
Vol 16 (3) ◽  
pp. 37-43
Author(s):  
Annarita Barbaro ◽  
Federica Napolitani Cheyne ◽  
Maria Cristina Barbaro
Keyword(s):  
Scholarly Publishing ◽  
Scientific Publishing ◽  
Academic Journals ◽  
Publishing Community ◽  
The Impact

This article proposes an analysis on the impact that COVID-19 pandemic is having on the process of scientific publishing in academic journals. It will specifically describe the response of the scholarly publishing community to meet the pressing demand from authors and researchers wishing to disseminate, as rapidly as possible, information on the virus. Its aim is to provide an overview for the community of librarians and information specialists about publishing in the COVID-19 era.

Impact Factor, My Donkey!

2010 ◽  
Vol 18 (1) ◽  
pp. 68-68
Author(s):  
Ray Egerton
Keyword(s):  
Impact Factor ◽  
Scientific Information ◽  
Scientific Publishing ◽  
The Impact

No recent phenomenon in scientific publishing is more remarkable than the rise of the Impact Factor (IF). Once an obscure statistic devised by the Institute for Scientific Information (ISI), it has now assumed a prominent place in the minds of researchers and administrators.

Formation of Lunar Craters and Bright Rays as a Result of Meteorite Impacts

1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten
Keyword(s):  
Explosive Charge ◽  
The Moon ◽  
Meteorite Impacts ◽  
The Earth ◽  
Lunar Craters ◽  
The Impact

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.

The Geosciences Applied to Lunar Exploration

1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green
Keyword(s):  
Lunar Surface ◽  
Probable Mechanism ◽  
Point Of View ◽  
Lunar Exploration ◽  
Geological Model ◽  
Apply Geophysics ◽  
Surface Features ◽  
The Impact

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.

Asteroid and Comet Impact Speeds upon Mars: Significance for Panspermia and the Supply of Organics

1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel
Keyword(s):  
Probability Distributions ◽  
Regions Of Interest ◽  
Significant Fraction ◽  
Organic Chemicals ◽  
Impact Speed ◽  
The Mean ◽  
The Impact

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.

Organic Syntheses During the Impact of a Comet with a Gaseous Planet

1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini
Keyword(s):  
Polymeric Material ◽  
Molecular Form ◽  
Parent Compound ◽  
Blue Filter ◽  
Organic Syntheses ◽  
The Impact

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.

Hydrogen Cyanide Polymers from the Impact of Comet P/Shoemaker-Levy 9 on Jupiter

1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman
Keyword(s):  
Amino Acids ◽  
Solar System ◽  
Hydrogen Cyanide ◽  
Nitrogen Heterocycles ◽  
Laboratory Studies ◽  
Heterogeneous Solids ◽  
The Many ◽  
Comet Halley ◽  
The Impact ◽  
By Products

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.

Unusual Microstructure in Shock-Compacted Graphite

1970 ◽  
Vol 28 ◽  
pp. 474-475
Author(s):  
Lucien F. Trueb
Keyword(s):  
Mechanical Characteristic ◽  
Compression Wave ◽  
Gray Zone ◽  
Flyer Plate ◽  
Compacted Graphite ◽  
The Impact

Crushed and statically compressed Madagascar graphite that was explosively shocked at 425 kb by means of a planar flyer-plate is characterized by a black zone extending for 2 to 3 nun below the impact plane of the driver. Beyond this point, the material assumes the normal gray color of graphite. The thickness of the black zone is identical with the distance taken by the relaxation wave to overtake the compression wave.The main mechanical characteristic of the black material is its great hardness; steel scalpels and razor blades are readily blunted during attempts to cut it. An average microhardness value of 95-3 DPHN was obtained with a 10 kg load. This figure is a minimum because the indentations were usually cracked; 14.8 DPHN was measured in the gray zone.

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